Novaya gazeta uchenyh dlya uchenyh
Vyshel devyatyi nomer obnovlennoi gazety
"Troickii variant"
Podpiska na rassylku obzorov astro-ph na Subscribe.Ru
Chislo podpischikov perevalilo 3300! Spasibo vam, druz'ya!
Soderzhanie i bystryi perehod k razdelam obzora
Fizicheskie usloviya v potencial'nyh istochnikah kosmicheskih luchei. I Novyi variant diagrammy Hillasa i ogranicheniya za schet radiacionnyh poter' Pervye izobrazheniya zatmennoi vzaimodeistvuyushei dvoinoi beta Liry Ochen' vysokotochnaya VLBI-astrometriya dlya pul'sara PSR J0437-4715 i prilozheniya k teoriyam gravitacii Obshii metod ocenki parametrov zvezd po dannym fotometrii
Otdel'nye stat'i
Iz razdela physics
Polnyi Arhiv predydushih vypuskov. Arhiv statei, voshedshih v vypuski s 01 iyulya 2002 g. po 31 marta 2003 g.
Arhiv na 14.04.2006
odnim failom
Razdely arhiva (s aprelya 2003 g.): Poleznye astronomicheskie ssylki. Korotkoe esse ob elektronnyh preprintah. Obzornye stat'i v astro-ph 2001-2003 gg.
Avtor proekta
Ranee uchastvovali:
Diskussii po stat'yam Arhiva
Proekt razmeshen na saitah:
Smotri takzhe diskussii i blogi:
Informacionnye partnery
Vy mozhet takzhe razmestit' na svoem saite nashu lentu obzorov Kniga avtora obzorov Novosti kosmonavtiki Novosti Nauchpopa Novosti ot UFN Informnauka Researcher@ Elementy.Ru Grani.Ru Perst Podpiska na rassylku obzorov na Subscribe.Ru
Druzhestvennye rassylki: "Astronomiya segodnya" "Okno vo Vselennuyu" Spisok astrorassylok |
Obzory preprintov astro-ph
Vypusk N192
astro-ph za 01 - 14 avgusta 2008 goda: izbrannye stat'i
Referaty otdel'nyh statei
Authors: F. Eisenhauer et al. Comments: 13 pages, 11 figures, to appear in the conference proceedings of SPIE Astronomical Instrumentation, 23-28 June 2008, Marseille, France Dlya VLT razrabatyvaetsya special'nyi pribor, kotoryi pomozhet nablyudat' dvizhenie zvezd i gaza v neposredstvennoi blizosti ot gorizonta sobytii v istochnike Sgr A* - sverhmassivnoi chernoi dyre v centre nashei Galaktiki. Dlya realizacii potrebuetsya ne tol'ko sozdat' novye instrumenty, no i zadeistvovat' vsyu mosh' interferometricheskoi sistemy VLT. Razumeetsya, nikto ne delaet pribor "pod odin ob'ekt", i v stat'e avtory rassmatrivayut i drugie vozmozhnye oblasti prilozhenii. Pribor nachnet rabotat' v 2013 godu (seichas ego sozdanie polnost'yu odobreno).
Authors: Bjoern Malte Schaefer Comments: 22 pages, 7 figures, invited review for IJMPD Galaktiki priobretayut uglovoi moment za schet prilivnyh vozdeistvii v processe formirovaniya krupnomasshtabnoi struktury. Razumeetsya, parametry vrasheniya okazyvayut skorrelirovany s drugimi parametrami galaktik i okruzhayushih ih struktur. Vse eto tak ili inache mozhet proyavlyat'sya v nablyudeniyah (v chastnosti, v dannyh po linzirovaniyu). Vsemu etomu i posvyashen dannyi obzor. Napisano otnyud' ne prosto.
Authors: J. Greiner, et al Comments: Excerpt of a proposal submitted in response to the ESA Cosmic Vision Call in June 2007, but not selected for further consideration; 11 pages, 6 Figs. only scientific sections Avtory predlagayut proekt novogo sputnika dlya izucheniya gamma-vspleskov. Osnovnaya novizna sostoit v vozmozhnosti spektroskopicheskih nablyudenii v shirokom diapazone (200 keV - 50 MeV) i v poluchenii dannyh o polyarizacii. Razumeetsya, takoi sputnik budet polezen ne tol'ko dlya issledovaniya gamma-vspleskov. Polnaya versiya prokta opublikovana v Experimental Astronomy.
Authors: Ksenia Ptitsyna, Sergey Troitsky Comments: 24 pages, 12 figures Ochen' vazhno pomnit', chto v "kosmicheskih uskoritelyah" chasticy ne tol'ko uskoryayutsya, no i izluchayut. Eto obstoyatel'stvo nakladyvaet ogranicheniya na maksimal'nye vozmozhnye energii. T.e., nel'zya prosto vzyat' diagrammu Hillasa (svyazyvayushuyu razmer i magnitnoe pole v istochnike kosmicheskih luchei) i poluchit' ocenku energii. Energiya na samom dele budet nizhe. A vot naskol'ko i pochemu - mozhno prochest' v obzore.
Authors: Paolo Lipari Comments: 31 pages, Talk given at the workshop "Neutrino Oscillations in Venice" (april 2008) Obzor posvyashen kosmicheskim lucham (a takzhe neitrino vysokih energii), tomu, kakuyu rol' ih issledovaniya zanimayut v astrofizike, i na kakie voprosy oni mogut pomoch' naiti otvety. Sm. takzhe obzor avtora arxiv:0808.0344.
Authors: Janusz Ziolkowski Comments: 13 pages, Chin. J. Astron. Astrophys. Vol. 8 (2008), Suppl., 273-280 Obsuzhdayutsya razlichnye metody ocenki mass dlya astrofizicheskih chernyh dyr (zvezdnyh, promezhutochnyh mass i sverhmassivnyh). Kak obychno v obzorah Ciolkovskogo, est' neskol'ko poleznyh tablic.
Authors: Reba M. Bandyopadhyay et al. Comments: 4 pages, 2 figures, to appear in the Proceedings of The Second Kolkata Conference on Observational Evidence for Black Holes in the Universe'', ed. S. Charkrabarti, Kolkata, India; AIP Conf. Series
Fantasticheski vyglyadit! Eto ne opticheskoe, a rentgenovskoe izobrazhenie.
Oblast' centra Galaktiki - vse nebo v almazah. Chandra vidit tam ob'ekty so
svetimost'yu do 1031 erg v sekundu.
Razumeetsya, otozhdestvlyat' istochniki v centre Galaktiki ochen' trudno. Tak chto
raboty tam eshe mnogo.
Authors: M. Zhao et al. Comments: 13 Pages, 3 Figures; Accepted by ApJL S pomosh'yu opticheskih interferometrov vpervye udalos' v detalyah razglyadet' sistemu betu Liry, razreshiv ee na dva komponenta.
Izobrazhenie polucheno s pomosh'yu sistemy CHARA Array. Vidna zvezda donor (sleva) i disk vokrug vtorogo komponenta. Vidno, chto donor slegka vytyanut, t.e. vpervye udalos' rassmotret' napryamuyu iskazhenie formy vo vremya zapolneniya polosti Rosha.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: Gary Steigman Comments: 4 pages, 1 figure Koroten'kaya zametka, posvyashennaya obsuzhdeniyu togo, kak rentgenovskie i gamma- nablyudeniya stalkivayushihsya skoplenii galaktik mogut dat' ogranicheniya na dolyu antiveshestva. Esli otbrosit' ideyu o tom, chto antiveshestvo s samyh rannih momentov zhizni vselennoi sobrano v kakie-to ochen' kompaktnye ob'ekty, to ogranicheniya na ego soderzhanie beretsya iz nablyudenii kosmicheskih luchei (nuzhno imenno zahvatyvat' chasticy, dlya etogo nuzhny sputniki tipa PAMELA) i nablyudenii gamma-luchei. Poslednie mogli by rozhdat'sya pri annigilyacii. Po gamma-izlucheniyu est' predely na dolyu antiveshestva na samyh raznyh masshtabah. Shteigman obsuzhdaet predely na masshtabah poryadka 10 Mpk - t.e. masshtabah skoplenii. Esli dva skopleniya stalkivayutsya (kak izvestnoe Bullet cluster), to antiveshestvo dolzhno annigilirovat' s veshestvom. Sootvetstvenno, verhnii predel na gamma-izlucheniya dast ogranichenie na antiveshestvo. Avtor rassmatrivaet konkretnye primery i obsuzhdaet, kak v budushem mozhno eshe uluchshit' takie predely.
Authors: David Blaschke, Thomas Klaehn, Fridolin Weber Comments: 16 pages, 11 figures, Contribution to Proceedings of the 3rd International Workshop on Astronomy and Relativistic Astrophysics (IWARA), 3-6 October 2007, Joao Pessoa, Brazil Ocherednoi obzor po astrofizicheskim ogranicheniyam na uravnenie sostoyaniya pri vysokoi plotnosti. Bystrovrashayushiesya i massivnye neitronnye zvezdy, kompaktnye ob'ekty s izmerennym radiusom, ochen' goryachie ili holodnye ... vse oni mogut dat' informaciyu o tom, kak vedet sebya veshestvo v ih nedrah pri plotnosti, v neskol'ko raz prevoshodyashei yadernuyu.
Authors: A. T. Deller, J.P.W. Verbiest, S.J. Tingay, M. Bailes Comments: 11 pages, 1 Figure, submitted to ApJL Avtory rasskazyvayut o tochnom opredelenii (tochnost' okolo 1%) parallaksa do samogo blizkogo (156 pk) millisekundnogo dvoinogo pul'sara i o tom, chto iz etogo mozhno izvlech'. A izvlech' mozhno nemalo, t.k. dlya takih ob'ektov est' nezavisimye metody opredeleniya rasstoyaniya. Eti nezavisimye metody osnovany na nekotoryh predpolozheniyah, kotorye mozhno proveryat', ispol'zuya tochnyi trigonometricheskii parallaks. Sredi etih prepolozhenii vo-pervyh nado otmetit' postoyanstvo postoyannoi tyagoteniya (n'yutonovoi). I avtory privodyat samyi zhestkii predel na ee proizvodnuyu. Vo-vtoryh, eto neizvestnye massivnye planety na zadvorkah solnechnoi sistemy. I v tret'ih, gravitacionno-volnovoi shum. Podrobnee ob izmerenii parallaksov pul'sarov s pomosh'yu VLBI sm. arxiv:0808.1598. V chastnosti, tam rasskazyvaetsya ob izmereniyah s submilliarksekundnoi tochnost'yu (tochno opredeleno rasstoyanie do pul'sara na ~2.5 kpc ot nas).
Authors: Elizabeth J. Tasker et al. Comments: 18 pages, 15 figures. Accepted for publication in MNRAS Avtory sravnivayut chetyre koda: Enzo, Flash, Gadget i Hydra. Dlya etogo oni reshayut s ih pomosh'yu nekotorye zadachi s izvestnymi resheniyami. Rech' ne idet o vyyavlenii "chempiona", prosto vazhno ponyat' kakie kody luchshe podhodyat dlya raznyh klassov zadach.
Authors: A.N. Belikov, S. Roser Comments: 14 pages, 20 figures, accepted by A&A Seichas est' mnogo horoshih obzorov neba s fotometricheskimi dannymi v shirokih polosah. Iz etih dannyh mozhno bylo by poprobovat' ocenit' parametery zvezd (effektivnye temperatury, metallichnost', silu tyazhesti), no ne vse tak prosto - est' mezhzvezdnoe veshestvo, kotoroe privodit k pokrasneniyu. Avtory predlagayut metod, kotoryi, po ih utverzhdeniyu, horosho spravlyaetsya s etoi neprostoi i aktual'noi zadachei. Sm. takzhe arxiv:0808.1848 ob absolyutnoi kalibrovke zvezd glavnoi posledovatel'nosti tonkogo diska po nablyudeniyam v optike i blizhnem IK.
Authors: S. Buitink et al. Comments: 8 pages, 8 figures, proceedings of XXth rencontres de Blois, 2008 Effekt Askaryana pozvolyaet registrirovat' vysokoenergichnye neitrino po radioizlucheniyu, kotoroe voznikaet pri dvizhenii chastic v srede. Na Zemle chashe obsuzhdayutsya ustanovki (i nekotorye uzhe rabotayut), gde "rabochim telom" sluzhit led (Antarkticheskii, grenlandskii). No Dagkesamanskii i Zheleznyh eshe v 1989 godu predlozhili nablyudat' s pomosh'yu radioteleskopov Lunu, i nablyudeniya byli provedeny. Pravda, udalos' poluchit' lish' verhnie predely. Rech' idet o registracii ochen' korotkih slabyh radiosignalov. V proekte NuMoon ispol'zuetsya bol'shoi teleskop v Vesterborke. Izyuminka v ispol'zovanii bolee nizkih chastot chem v predydushih popytkah. Nablyudeniya uzhe nachalis'. Rezul'taty poka pozvolyayut lish' postavit' verhnie predely, no eto uzhe ochen' horoshie predely.
My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing).
Authors: Ariel Caticha Comments: 170 pages. Invited lectures at MaxEnt 2008, the 28th International Workshop on Bayesian Inference and Maximum Entropy Methods in Science and Engineering (July 8-13, 2008, Boraceia Beach, Sao Paulo, Brazil) 170 stranic lekcii.... Mnogo teorem s dokazatel'stvami. No s drugoi storony mnogo i primerov primenenii raznyh statisticheskih metodov.
Authors: Lawrence M. Krauss Comments: to appear in "Physics in Canada", response to 0807.3670 Ya pisal o zametke arxiv:0808.3670. Ona byla naveyana vystupleniem Kraussa. Teper' Krauss pis'menno otvechaet na nee. Krauss pishet, chto vcelom on soglasen s avtorom arxiv:0807.3670, a razlichiya u nih v osnovnom terminologicheskie.
Authors: L.B. Okun Comments: 20 pages, Published: Uspekhi Fiz. Nauk 178 (5) (2008) 541-555 (in Russian); Physics--Uspekhi 51 (5) (2008) 513-527 (in English) Obsuzhdaetsya izvestnaya formula E=mc^2, rol' indeksa "0" u energii i koe-chto eshe.
Na russkom stat'yu mozhno skachat'
tut.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: A.A. Tseytlin Comments: 38 p., 21 fig Nazvanie govorit samo za sebya, no uchtite, chto tekst sostoit prakticheski tol'ko iz odnih formul.
Authors: W. C. Haxton Comments: 37 pages, 15 figures; presentation at an introductory level Horoshii obzor po vsem oblastyam neitrinnoi astrofiziki: solnechnye neitrino, atmosfernye, ot sverhnovyh, rol' neitrino v nukleosinteze, processy v zvezdah, neitrino vysokih energii. Razumeetsya, perechisleny osnovnye ustanovki i plany v etoi oblasti. Vse zhostatochno polno i ponyatno. Rekomenduyu.
|
Publikacii s klyuchevymi slovami:
astro-ph - elektronnye preprinty
Publikacii so slovami: astro-ph - elektronnye preprinty | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> |