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Referaty otdel'nyh statei
Authors: Edward M. Cackett, et al. Comments: 5 pages, 3 figures, 3 tables, submitted to ApJL Avtory opisyvayut nablyudeniya na sputnike Suzaku. Cel'yu bylo issledovanie linii zheleza v spektrah malomassivnyh rentgenovskih dvoinyh. Izuchenie etih linii mozhet pozvolit' dat' sushestvennye ogranicheniya na radiusy neitronnyh zved. Ideya v tom, chtoby detal'no rassmotret' linii, ispuskaemye s vnutrennego kraya akkrecionnogo diska. Yasno, chto razmer neitronnyi zvezdy men'she. Poskol'ku dlya nekotoryh malomassivnyh rentgenovskih dvoinyh vnutrennii krai diska podbiraetsya ochen' blizko k poverhnosti kompaktnogo ob'ekta, mozhno postavit' horoshii verhnii predel na razmer neitronnoi zvezdy. Predely sootvetstvuyut radiusam poryadka 14.5-16.5 km, esli predpolozhit', chto massy neitronnyh zvezd ravny 1.4 solnechnyh. Sm. takzhe arxiv:0708.3648, gde rech' idet o nablyudenii linii zheleza ot odnogo iz ob'ektov, popavshem v lenty novostei. I arxiv:0708.3816, gde primenyaetsya drugoi podhod dlya ogranicheniya razmerov i mass neitronnyh zvezd na osnove ih rentgenovskih spektrov.
Authors: Michael T. Murphy, John K. Webb, Victor V. Flambaum Comments: 1 page, 1 EPS figure. Submitted as a PRL Comment on arXiv:astro-ph/0402177 . Further details available in arXiv:astro-ph/0612407 V poslednie gody aktivno obsuzhdaetsya potencial'naya vozmozhnost' opredeleniya vremennyh variacii postoyannoi tonkoi struktury iz analiza absorbcionnyh linii v spektrah kvazarov vysokogo razresheniya. Odnako sovremennyi uroven' tochnosti, dostizhimyi teleskopami Keck/HIRES i VLT/UVES, poka ne pozvolyaet odnoznachno razreshit' etot vopros. V dannoi zametke zakryvaetsya sensacionnoe soobshenie, opublikovannoe ranee v astro-ph/0402177, o dostignutoi tochnosti $\Delta\alpha/\alpha=(-0.06\pm0.06)\times10^{-5}$. Na osnove bolee korrektnoi statisticheskoi obrabotki teh zhe nablyudatel'nyh dannyh avtorami zametki dokazano, chto uroven' tochnosti na segodnya ne mozhet byt' principial'no luchshe, chem $\Delta\alpha/\alpha=(-0.44\pm0.16)\times10^{-5}$. Podrobnyi analiz rezul'tatov opublikovan v astro-ph/0612407.
Authors: J. A. Irwin, H. Kennedy , T. Parkin, S. Madden Comments: 16 pages, 5 gif figures, accepted for publication in A&A Uzhe mnogo let priroda diffuznyh polos, voznikayushih v mezhzvezdnoi srede, ostaetsya zagadkoi. Odno iz vozmozhnyh ob'yasnenii - policiklicheskie aromaticheskie uglevody (Polycyclic Aromatic Hydrocarbonc ili PAHs) - pylevye chasticy slozhnoi struktury. Galaktika NGC 5529, vidimaya s rebra, nablyudalas' avtorami v polose 6.7 mkm, v kotoroi izluchenie PAHs preobladaet. Bylo naideno protyazhennoe strukturirovannoe galo, prostirayusheesya do vysot 3.7 kps nad ploskost'yu galaktiki, i sledovatel'no sushestvuet process, pozvolyayushii vynosit' pylevye chasticy daleko za predely diska galaktik. Eto uzhe vtoroi sluchai izucheniya galo galaktiki v izluchenii PAHs (NGC 5907). Nuzhno otmetit', chto galaktiki vidimye s rebra seichas aktivno nablyudayutsya na mnogih dlinah voln. Kazhdaya iz komponent mezvezdnoi sredy (pyl' i PAHs, molekulyarnyi i neitral'nyi gaz, diffuznyi ionizovannyi gaz) neset vazhnuyu informaciyu o slozhnyh pocessah vzaimodeistviya diska i galo, pomogaet ponyat' prirodu galakticheskogo vetra, proyasnyaet detali himicheskoi evolyucii.
Authors: LIGO Scientific Collaboration: B. Abbott, et al Comments: 39 pages, 41 figures Privedeny dannye obrabotki ocherednogo (chetvertogo) otrezka nauchnoi raboty gravitacionno-volnovoi antenny LIGO. Eto byl dostatochno korotkii progon - okolo mesyaca - v nachale 2005 goda. No vazhno ponimat', chto obrabotka dannyh zanimaet ochen' bol'shoe vremya! Avtory obsuzhdayut poiski periodicheskogo signala. Nichego ne naideno, no predely (osobenno dlya nekotoryh uchastkov nebesnoi sfery) stanovyatsya uzhe interesnymi.
Authors: Roger Cayrel, et al. Comments: Accepted for publication on A&A Letters Litii - sovershenno unikal'nyi himicheskii element, sostoyashii iz dvuh izotopov 6Li i 7Li. Sintez litiya proishodit tremya spososobami: srazu posle Bol'shogo Vzryva v processe pervichnogo nukleosinteza (tol'ko 7Li), v processe zvezdnoi evolyucii na stadii AGB - asimptoticheskoi vetvi gigantov (tol'ko 7Li) i pri vzaimodeistvii kosmicheskih luchei s atomami mezhzvezdnoi sredy (v osnovnom 6Li). Poskol'ku 6Li sinteziruetsya gorazdo pozzhe 7Li, otnoshenie izotopov litiya 6Li/7Li v staryh malometallichnyh zvezdah galo sluzhit odnim iz vazhnyh nablyudatel'nyh testov teorii pervichnogo nukleosinteza. Avtory dannoi stat'i (polovina iz nih - vsemirno izvestnye uchenye) dvumya razlichnymi sposobami izuchili soderzhanie izotopov litiya v atmosfere malometallichnoi zvezdy HD 74000, prinadlezhashei galo nashei Galaktiki. Rezul'taty etogo analiza, osnovannogo na novom metode razdeleniya blendirovannyh linii izotopov 6Li i 7Li, pokazali, chto dlya vseh ranee opublikovannyh rabot mozhno s bol'shoi uverennost'yu govorit' o sistematicheskoi pereocenke soderzhaniya izotopa 6Li. Po ocenke avtorov, soderzhanie 6Li v atmosfere zvezdy HD 74000 (metallichnost' [Fe/H]=- 2.0 dex) ne prevyshaet odnogo-dvuh procentov ot soderzhaniya izotopa 7Li. Esli rezul'tat podobnogo analiza budet podtverzhden dlya statisticheski znachimogo chisla malometallichnyh zvezd, ischeznet neobhodimost' poiska variantov sinteza 6Li na rannih etapah evolyucii Vselennoi i nablyudatel'noe ogranichenie teorii pervichnogo nukleosinteza budet nadezhno podtverzhdeno.
Authors: Ilian T. Iliev, Paul R. Shapiro , Garrelt Mellema, Ue-Li Pen, Patrick McDonald, J. Richard Bond Comments: 3 pages, to appear in the Proceedings of First Stars III, Santa Fe, July 2007, AIP Conf. Series Reionizaciya - sravnitel'no nedolgii etap evolyucii Vselennoi ot momenta obrazovaniya pervyh zvezd na z= 30-40, kogda mezhgalakticheskaya sreda byla polnost'yu neitral'noi i holodnoi, do momenta, sootvetsvuyushego krasnym smesheniyam z=6-7, kogda MGS stala ionizovannoi i goryachei. Progress v ponimanii prirody i svoistv etogo nedostupnogo pryamomu izucheniyu perioda dostignut v poslednie gody blagodarya sovremennym kosmologicheskim nablyudatel'nym proektam i modelirovaniyu perenosa izlucheniya v usloviyah rannei Vselennoi. V zametke Iliana Il'eva dano dostupnoe ne kosmologam izlozhenie osnovnyh faktov o reionizacii. Eta nebol'shaya stat'ya (i glavnoe ssylki v nei) mozhet byt' poleznoi dlya pervogo oznakomleniya s temoi, kotoraya stanovitsya vse bolee i bolee populyarnoi.
Authors: Falk Herwig Comments: Biermann award 2004 lecture, AG meeting, Prague (2005RvMA...18...21) "Vtorye zvezdy" - eto svetila, voznikshie srazu posle pervyh. Pervye sostoyali tol'ko iz pervichnogo veshestva, poetomu v osnovnom byli ochen' massivnymi i zhili nedolgo. Seichas takih net (esli, konechno, gde-to ne ostalos' dostatochnoe kolichestvo ploho peremeshannogo gaza). "Vtorye zvezdy" obrazovyvalis' iz uzhe slegka obogashennogo tyazhelymi elementami veshestva. Poetomu oni mogli byt' malomassivnymi, a znachit mogli dozhit' do nashih dnei. T.o., oni yavlyayutsya unikal'nymi "svidetelyami epohi". O tom, chto oni rasskazyvayut nam - v stat'e.
Authors: Paolo Molaro Comments: talk given at the conference "Pathways Through an Eclectic Universe" Johan Knapen, Terry Mahoney and Alexandre Vazdekis Editors V paru k predydushemu obzoru mozhno porekomendovat' stat'yu po pervichnomu soderzhaniyu legkih elementov vo vselennoi (sm. takzhe vyshe stat'yu 0708.3819).
Authors: Stephen C. Unwin et al. Comments: 54 pages, 28 figures, uses emulateapj. Submitted to PASP Chto zh, lyudi hotyat imet' parallaksy s tochnost'yu 4 mikrosekundy dugi dlya ob'ektov do 20 zvezdnoi velichiny. Ozhidaetsya, chto sputnik SIM PlanetQuest smozhet eto delat'. Avtory obsuzhdayut, kakie novye rezul'taty mozhno poluchit' s pomosh'yu takogo instrumenta.
Authors: Joseph L. Hora Comments: 8 pages, 2 figures, invited review to appear in the proceedings of the conference "Asymmetrical Planetary Nebulae IV", eds. R.L.M. Corradi, A. Manchado & N. Soker Nebol'shaya stat'ya, v kotoroi dana svodka dannyh po planetarnym tumannostyam, poluchennyh na kosmicheskom infrakrasnom teleskope imeni Spitcera. Drugoi poleznyi korotkii obzor iz togo zhe sbornika (uzhe yasno, chto takim miniobzorov budet mnogo) posvyashen asimmetrii planetarnyh tumannostei.
Authors: Raphael Bousso Comments: 39 pages, 3 figures Obzornye lekcii po kosmologicheskoi postoyannoi. Obozrevayutsya raznye aspekty, vklyuchaya vozmozhnye puti resheniya problemy v ramkah teorii strun.
Authors: Simon Johnston, M. Kramer, A. Karastergiou, G. Hobbs, S. Ord, J. Wallman Comments: Accepted by MNRAS. 14 pages Avtory privodyat dannye po polyarizacionnym issledovaniyam 22 pul'sarov. Osnovnyh rezul'tatov dva. Vo-pervyh, dlya nekotoryh iz neitronnyh zvezd udalos' ocenit' ugol mezhdu os'yu vrasheniya i napravleniem prostranstvennoi skorosti. Vo-vtoryh, avtory smogli sdelat' ocenki vysoty nad poverhnost'yu neitronnoi zvezdy, na kotoroi ispuskaetsya izluchenie v raznyh fazah. Ugly ocenili dlya 14 pul'sarov. U semi iz nih oni dostatochno maly. Eto nahoditsya v soglasii s bolee rannimi rezul'tatami na men'shei statistike (hotya, ranee polagali, chto u vseh oni mogut byt' maly). Chto kasaetsya vysot izlucheniya, to, opyat' zhe v soglasii s bolee rannimi dannymi, chto izluchenie v seredine profilya impul'sa generiruetsya na bolee nizkih vysotah, chem po krayam profilya.
Authors: Attilio Anselmo Comments: 6 pages, 7 figures Lyubopytnaya zametka. Avtor, proanalizirovav pyl' s krysh domov, pokazyvaet, chto sfericheskie chasticy, kotorye inogda svyazyvayut s mikrometeoritami, na samom dele svyazany s tehnicheskoi deyatel'nost'yu cheloveka.
Authors: Andrei Lobanov Comments: Invited review at the 8th European VLBI NetworkSymposium. 12 pages, 6 figures, PoS tex. To be published electronically by Proeedings of Science Kompaktnyi obzor po kompaktnym radiodzhetam. Dana ochen' horoshaya svodka dannyh.
Authors: Judith G. Cohen,et al. Comments: Accepted to the ApJ Avtorami predstavlen detal'nyi analiz spektrov vysokogo razresheniya novyh vos'mi zvezd galo nashei Galaktiki, imeyushih predel'no malye metallichnosti [Fe/H] < -3.5 dex. Pohozhe na to, chto pri ochen' malyh metallichnostyah stohastichnost' vzryvov sverhnovyh II i neeffektivnost' peremeshivaniya mezhzvezdnoi sredy okazyvayut sushestvennoe vliyanie na nablyudaemye otnositel'nye soderzhaniya himicheskih elementov v atmosferah etih zvezd. Dannye takogo roda yavlyayutsya vazhnym istochnikom informacii o nachal'nyh stadiyah evolyucii Galaktiki, a takzhe sluzhat testom dlya zvezdnoi teorii nukleosinteza.
Authors: Rudy Wijnands et al. Comments: submitted to MNRAS Pohozhe, chto odin iz gamma-vspleskov na samom dele yavlyaetsya neobychnoi vspyshkoi na neitronnoi zvezde v tesnoi dvoinoi sisteme. Avtory polagayut, chto ne isklyucheno, chto est' mnogo sistem takogo tipa, no poka oni uskol'zayut ot nablyudatelei iz-za trudnoulovimosti ih vspyshek.
Authors: V. I. Dokuchaev, Yu. N. Eroshenko, S. G. Rubin Comments: 42 pages, 5 figures, review paper Dan obzor razlichnyh scenariev obrazovaniya sverhmassivnyh chernyh dyr. Razumeetsya, avtory obsuzhdayut nedostatki razlichnyh scenariev i vozmozhnye puti resheniya imeyushihsya problem.
Authors: O. Steiner Comments: 48 pages, 33 figures, Lecture notes Lekcii posvyasheny processam v poverhnostnyh sloyah Solnca. Dannye nablyudenii pokazyvayut inteersnye melkomasshtabnye struktury. S pomosh'yu chislennogo modelirovaniya udaetsya ponyat', chto zhe my nablyudaem.
Authors: F. Combes Comments: 10 pages, 6 figures, review paper in the Proceedings of the IAU Symposium 245, "Formation and Evolution of Galaxy Bulges", held at Oxford, U.K., July 2007 Obsuzhdaetsya vliyanie radial'nyh gazovyh techenii na dinamiku spiral'nyh galaktik. Rassmatrivaetsya ih vliyanie na processy, proishodyashiev central'nyh oblastyah galaktik.
Authors: S. Ekstroem, G. Meynet, A. Maeder Comments: to be published in the conference proceedings of First Stars III, Santa Fe, 2007 Massivnye zvezdy maloi metallichnosti v nekotorom diapazone mass dolzhny teryat' svoyu ustoichivost' iz-za rozhdeniya par v yadre, chto privodit k specificheskomu vzryvu sverhnovoi. Takie sverhnovye dolzhny ostavlyat' harakternye "otpechatki pal'cev" iz-za osobennostei sostava vybrasyvaemogo veshestva. "Uliki" ne obnaruzheny. Eto mozhet byt' svyazano s tem, chto vse-taki takie vzryvy ne proishodyat. Avtory rassmatrivayut nekotorye varianty, dlya togo, chtoby zvezdy mogli izbezhat' takoi neustoichivosti. Pohozhe, chto variant naiden.
Authors: Robert M. Quimby et al. Comments: ApJ Letters Accepted; 4 pages Opisany nablyudeniya samoi moshnoi sverhnovoi, vspyhnuvshei v 2005 godu. Blagodarya sisteme ROTSE-III ee udalos' nablyudat' i do maksimuma bleska.
Authors: K. M. Menten et al. Comments: 13 pages, 3 figures, to appear in Astronomy & Astrophyiscs S pomosh'yu VLBA izmeren trigonometricheskii parallaks dlya neskol'kih chlenov skopleniya v tumannosti Oriona. Rasstoyanie ravno 414+/-7 pk.
Authors: Irit Maor, Lawrence Krauss, Glenn Starkman Comments: 13 pages Avtory privodyat dostatochno ubeditel'noe rassuzhdenie v pol'zu togo, chto ne stoit vosprinimat' fakt nashego sushestvovaniya kak nechto bezuslovno ob'yasnyayushee velichinu kosmologicheskoi postoyannoi. Naprimer, pri podobnom ob'yasnenii molchalivo predpolagaetsya, chto my yavlyaemsya tipichnymi nablyudatelyami, chto ne ochevidno.
Authors: Massimo Ricotti, Jeremiah P. Ostriker, Katherine J. Mack Comments: 17 pages (Apj style), 9 figures, submitted to ApJ Avtory obsuzhdayut, kak nalichie dostatochno massivnyh (ne isparayushihsya) pervichnyh chernyh dyr mozhet vliyat' na svoistva reliktovogo izlucheniya, reionizaciyu i tp. Udaetsya dat' sushestvenno (na poryadki) bolee strogii predel na chernye dyry s massoi bolee 0.1 solnechnoi. Uchet pervichnyh chernyh dyr dostatochno bol'shoi massy mozhet byt' vazhen pri opredelenii kosmologicheskih parametrov (ved' pri takoi procedure vsegda zakladyvaetsya nekotoraya model').
Authors: Mitchell C. Begelman Comments:5 pages, 2 figures. To appear in "First Stars III", proceedings of the conference in Santa Fe, NM, July 16-20, 2007, eds. B. O'Shea, A. Heger and T. Abel. AIP Conference Proceedings Avtor rassmatrivaet bystroe formirovanie chernyh dyr v yadrah galaktik za schet pryamogo kollapsa gaza (t.e. bez obrazovaniya zvezd). Za schet akkrecii takie dyry bystro narashivayut svoyu massu do neskol'kih tysyach solnechnyh. Eto mozhet pomoch' reshit' problemu bystrogo rosta massy sverhmassivnyh chernyh dyr.
Authors: Craig J. Hogan Comments: 10 pages, LaTeX, to appear in "Frontiers of Astrophysics: A Celebration of NRAO's 50th Anniversary", eds. A.H.Bridle, J.J.Condon and G.C.Hunt Avtor rassmatrivaet, kakie vozmozhnosti v issledovanii vselennoi otkroyutsya pered nami v blizhaishie desyatiletiya za schet pryamoi registracii gravitacionnyh voln.
Authors: V.A. McBride et al. Comments: Accepted for publication in MNRAS Opisany rezul'taty dovol'no staryh (2003 god) nablyudenii Malogo Magellanovogo oblaka na sputnike Integral. Pribory uvideli dva istochnika. Odin iz nih chetko otozhdestvlyaetsya kak izvestnaya sistema SMC X-1. Vtoroi istochnik ne otozhdestvlen. Vozmozhno, chto eto ranee neizvestnaya rentgenovskaya dvoinaya (skoree vsego rentgenovskii pul'sar s massivnym kompan'onom i akkreciei cherez vnutrennyuyu tochku lagranzha).
Authors: H. Krawczynski et al. Comments: 4 pages, Proceedings of the 30th ICRC, Merida, Mexico, July 2007 V svyazi s burnym razvitiem nazemnoi gamma-astronomii astrofizicheskoe podrazdelenie Amerikanskogo fizicheskogo obshestva zakazalo podorbnyi otchet (t.n. "beluyu knigu") po etoi teme. V korotkoi zametke avtory opisyvayut rabotu gruppy, zanimayusheisya sostavleniem otcheta.
Authors: Frederic Zagury Comments: accepted for publication in Astrophysics and Space Science. 16 pages, 12 figures. Provedennyi avtorom analiz nablyudatel'nyh dannyh pokazal, chto zakony poglosheniya v nashei Galaktike, Bol'shom i Malom Magellanovom oblakah imeyut odinakovuyu prirodu i, sledovatel'no, net neobhodimosti v predpolozhenii o tom, chto svoistva pylevyh chastic v etih galaktikah sil'no otlichayutsya drug ot druga. S tochki zreniya avtora sovremennyi uroven' znaniya ne pozvolyaet vydelit' i opisat' takie razlichiya.
Authors: Ryan Scranton et al. Comments: 10 pages, 3 figures, to be submitted to PASP Opisan proekt Sky in Google Earth. Bol'she skazat'-to i nechego!
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: LIGO Scientific Collaboration Comments: 23 pages, 10 figures, 14 tables; to be submitted to Phys. Rev. D Po dannym treh etapov nauchnoi raboty LIGO postavleny verhnie predely na gravitacionnoe izluchenie ot 39 gamma-vspleskov.
Authors: Gustavo Medina-Tanco, for the Pierre Auger Collaboration Comments: Proc. of the 30th Int. Cosmic Ray Conference, Merida, Mexico, July 2007 Dlya yuzhnoi (argentinskoi) chasti observatorii imeni P'era Ozhe zaplanirovan vvod v stroi novyh detektorov. Kak ni stranno, no cel'yu yavlyaetsya ne dvizhenie v storonu registracii bolee energichnyh kosmicheskih luchei, a naoborot. Delo v tom, chto luchi s energiei menee 1018 eV registriruyutsya ne slishkom horosho. Ved' iznachal'noi cel'yu byli imenno luchi sverhvysokih energii! Teper' uchenye hotyat protyanut' chuvstvitel'nost' priborov v storonu bolee nizkih energii (razumeetsya, sdelat' eto gorazdo proshe, chem povyshat' veroyatnost' registracii bolee energichnyh chastic). Novovvedenie pozvolit izuchat' na observatorii oblasti spektra, nazyvaemye "vtorym kolenom" i "lodyzhka" (iznachal'no byl vveden termin "koleno", otrazhayushii izlom v spektre). Bezuslovno, ochen' vazhno poluchat' dannye v dostatochno shirokom diapazone v ramkah odnogo i togo zhe eksperimenta.
Authors: M.Cantiello, S.-C.Yoon, N.Langer, M.Livio Comments: 6 pages, To appear in the proceedings of the conference "Unsolved problems in stellar physics" - Cambridge, July 2007 Dlya poyavleniya dlinnogo gamma-vspleska, chto v naibolee populyarnom scenarii svyazyvaetsya s kollapsom yadra dostatochno massivnoi zvezdy, neobhodimo bystroe vrashenie yadra zvezdy. Obychno zvezdy dostatochno effektivno zamedlyayutsya. Raskrutit' zvezdu mozhno v tesnoi dvoinoi sisteme. Krome togo, bylo predlozheno, chto pri maloi metallichnosti zvezdy ostayutsya dostatochno bystrovrashayushimisya. V dannoi stat'e predstavlen analiz situacii, v kotoroi malometallichnaya zvezda vhodit v tesnuyu dvoinuyu sistemu. Vo-pervyh, pokazano, chto v takoi dvoinoi mozhno poluchit' usloviya, pri kotoryh vtoraya (menee massivnaya) zvezda dast gamma-vsplesk. Vo-vtoryh, sistema raspadaetsya posle pervogo vzryva, poetomu mozhno ozhidat', chto predsverhnovaya budet ubegayushei zvezdoi. Eto znachit, chto ona proidet neskol'ko sot parsek do porozhdeniya vspleska. Nakonec, poskol'ku skoree vsego napravlenie dzheta budet perpendikulyarno skrosti zvezdy , mozhno sdelat' predskazaniya otnositel'no svoistv sredy vokrug vzryvayusheisya zvezdy. Eto vazhno dlya opisaniya svoistv poslesvechenii (oreolov) gamma-vspleskov.
Authors: Daniel J. Price Comments: 14 pages, 11 figures, accepted to PASA Avtor opisyvaet (i reklamiruet) soft dlya vizualizacii gidrodinamicheskih raschetov metodom sglazhennyh chastic. Programma dostupna dlya skachivaniya.
Authors: Nikos Prantzos Comments: 46 pages, 25 figures, an introductory course to appear in "Stellar Nucleosynthesis: 50 years after B2FH", C. Charbonnel and J.P. Zahn (Eds.), EAS publications Series Bol'shoi obzor vvodnogo haraktera po himicheskoi evolyucii Galaktiki.
Authors: N. R. Tanvir, A. J. Levan Comments: 10 pages, 4 figures, to appear in proceedings of 070228: The next decade of GRB afterglows, Amsterdam March 2007 Dlya mnogih gamma-vspleskov my mozhem poluchit' vpolne podrobnuyu informaciyu o galaktikah, v kotoryh oni poyavilis'. Razumeetsya, eto daet mnogo povodom dlya razdumii. Avtory rezyumiruyut nashe znanie v etoi oblasti, i pytayutsya pokazat', kak eto pomogaet v ponimanii prirody mehanizma vspleskov.
My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing).
Authors: U. Kraus Comments: To be published in The European Journal of physics, 13 pages, 9 figures, for associated mpeg files see this http URL (section "First-person visualizations of the special and general theory of relativity") Avtor predlagaet animacii effektov STO i OTO. Stat'ya soderzhit nekotorye neobhodimye poyasneniya.
Authors: Paolo Di Vecchia, Adam Schwimmer Comments: Latex 18 pages, 3 figures, use svmult.cls. Contribution to the volume "String theory and fundamental interactions", dedicated to Gabriele Veneziano on his 65th birthday Pervye raboty po tomu napravleniyu, kotoroe pozzhe prevratilos' v teoriyu strun, prinadlezhat izvestneishemu fiziku-teoretiku Gabriele Veneciano. K ego yubileyu (tradicionno v mire otmechayut 65-letie uchenyh, prichina etogo budet maloponyatna bol'shinstvu nashih nachal'nikov, zanimayushih svoi posty pozhiznenno) Veneciano i napisan nebol'shoi obzor po rannim rabotam v teorii strun.
Authors: Frank Wilczek Comments: 20 pages, no figures Neprostoi, no ochen' soderzhatel'nyi tekst ot Franka Vil'cheka.
Authors: B. Ananthanarayan, Kshitij Garg Comments: 6 pages, submitted to Current Science Avtory rassmatrivayut neskol'ko nedavnih eksperimentov (BELLE na KEK-B v Yaponii i KLOE na ustanovke DAFNE v Italii), v kotoryh bylo podtverzhdeno nablyudenie zaputyvaniya sostoyanii, a takzhe podtverzhdena t.n. CPT-teorema.
Authors: F. Petrelis, N. Mordant, S. Fauve Comments: 40 pages, 13 figures V astrofizike generaciya polya razlichnymi dinamo-mehanizmami igraet ogromnuyu rol'. Okazyvaetsya, i v laboratorii mozhno pytat'sya vosproizvesti takoi process. V stat'e opisyvaetsya tri uspeshnyh eksperimenta i obsuzhdayutsya ih rezul'taty.
Authors: Hiroyasu Tajima Comments: 14 pages, 21 figures, Invited Talk at 11th Vienna Conference on Instrumentation, Vienna, Austria, February 19-24, 2007, To be published in Nuclear Instruments and Methods A Avtor daet obzor sovremennyh eksperimentov v oblasti kosmicheskih luchei: observatoriya im. Ozhe, PAMELA, ICECUBE, ANITA, rassmatrivaet cherenkovskie teleskopy (CANGAROO, HESS, MAGIC, VERITAS), zatem rech' idet o sputnike GLAST.
Authors: Daniel Kennefick Comments: 30 pages, to appear in proceedings of the 7th Conference on the History of General Relativity, Tenerife, 2005 Avtor rassmatrivaet vazhnyi moment v istorii nauki: ekspediciyu 1919 goda, v hode kotoroi proveryalos' predskazanie OTO ob otklonenii luchei sveta v pole Solnca. Vyvod avtora v tom, chto nablyudateli ne byli predvzyaty, t.e., chto oni ne stremilis' podtverdit' OTO, a provodili normal'noe neangazhirovannoe issledovanie.
Authors: Bruno Preziosi, Erasmo Recami Comments: bilingual submission of 34 pages: (i) article in English (16 pages), and (ii) article in Italian (18 pages). Edited, "finished" versions of these papers appeared as: Journal-ref: chapter 11 in "Ettore Majorana - Scientific Papers", ed. by G.F.Bassani and SIF (S.I.F. and Springer; Bologna and Berlin, 2006) Ocherednaya stat'ya, posvyashennaya rabote izvestnogo ital'yanskogo fizika i matematika Ettore Maiorany. V stat'e privodyatsya zametki, podgotovlennye im dlya lekcii v Neapole.
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