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Testy gravitacii v sil'nom pole s pomosh'yu nablyudenii elektromagnitnyh voln Ochen' massivnaya dvoinaya NGC3603-A1 Porazitel'nye razlichiya mezhdu molodymi zvezdami-bliznecami v dvoinoi sisteme Astrofizicheskie prilozheniya gipoteticheskih stabil'nyh TeVnyh chernyh dyr
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
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Razdely arhiva (s aprelya 2003 g.): Poleznye astronomicheskie ssylki. Korotkoe esse ob elektronnyh preprintah. Obzornye stat'i v astro-ph 2001-2003 gg.
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astro-ph za 10 - 23 iyunya 2008 goda: izbrannye stat'i
Referaty otdel'nyh statei
Authors: Rodrigo F. Daz et al. Comments: Accepted for publication in ApJ Letters Avtory obnaruzhili periodicheski otkloneniya v dvizhenii odnoi iz vnesolnechnyh planet. Edinstvennym vozmozhnym ob'yasneniem, po mneniyu avtorov, yavlyaetsya vliyanie planety s massoi poryadka zemnoi. Soobsheniya o novyh otkrytiyah tranzitnyh planet s massoi v neskol'ko yupiterianskih mozhno naiti zdes': arxiv:0806.1478, arxiv:0806.1482.
Authors: Brian Warner, Patrick A. Woudt Comments: 10 pages, 7 figures, to appear in Cool discs, hot flows: The varying faces of accreting compact objects' (AIP Conf. Series) Daetsya obzor po razlichnym kvaziperiodicheskim processam, nablyudaemym u kataklizmicheskih peremennyh. Krome razlichnyh processov, svyazannyh s diskovoi akkreciei, v takih sistemah dobavlyaetsya vozmozhnost' nalichiya neradial'nyh pul'sacii belyh karlikov.
Authors: Dimitrios Psaltis Comments: 58 pages, review article for Living Reviews in Relativity Avtor podrobno obsuzhdaet razlichnye vozmozhnosti dlya izucheniya gravitacionnyh effektov v sil'nom pole po nablyudeniyam neitronnyh zvezd i chernyh dyr. Obzor ochen' dostupen, no pri etom avtor kasaetsya vseh osnov.
Authors: Stanislav Babak, Mark Hannam, Sascha Husa, Bernard Schutz Comments: 4 pages, 1 figure Kosmicheskii lazernyi interferometr LISA budet registrirovat' sliyaniya sverhmassivnyh chernyh dyr. Sprashivaetsya, mozhem li my dostatochno tochno opredelit', v kakoi galaktike proizoshlo sliyanie? Avtory pokazyvayut, chto s uchetom togo, chto my mozhem rasschitat', kak dolzhen vyglyadet' signal (i ot samogo sliyaniya i t.n. "zvon" posle nego), polozhenie mozhno budet opredelyat' dostatochno tochno. Dlya poloviny sistem na z=1 polozhenie budet opredelyat'sya s tochnost'yu 3 uglovye minuty, a dlya 20 procentov - odna uglovaya minuta.
Authors: Martha P. Haynes Comments: To appear in AIP Conference Proceedings, "The Evolution of Galaxies through the Neutral Hydrogen Window", Feb 1-3 2008, Arecibo, Puerto Rico, eds. R. Minchin & E. Momjian. 8 pages V Arhive potihon'ku poyavlyayutsya stat'i, kotorye budut opublikovany v materialah konferencii po izucheniyu neitral'nogo vodoroda. Eti issledovaniya vazhny dlya ponimaniya processa formirovaniya galaktik, nekotoryh kosmologicheskih aspektov. O proekte ALFALFA (The Arecibo Legacy Fast ALFA) mozhno prochest' tut arxiv:0806.1670. V ego ramkah provoditsya obzor vnegalakticheskogo neitral'nogo vodoroda (razumeetsya, rech' idet o volne 21 sm). Na nastoyashii moment zakoncheno bolee poloviny nablyudatel'noi raboty i okolo chetverti raboty po obrabotke dannyh. Ob istorii i rezul'tatah issledovaniya blizkih galaktik na volne 21 sm sm. arxiv:0806.1712. Razumeetsya, na radioteleskope v Aresibo, kotoryi seichas igraet vedushuyu rol' v issledovanii galaktik na volne 21sm, planiruyutsya novye nablyudeniya. Pro to napisano zdes' arxiv:0806.1714.
Authors: I. Dilmann, the JINA-CARINA Collaboration Comments: Proceedings 10th Int. Symp. on Origin of Matter and Evolution of Galaxies OMEG07, Sapporo/Japan, December 4-7 2007 Dlya raschetov processov v zvezdah, v rannei vselennoi, pri vzryvah sverhnovyh i tak dalee neobhodimy dannye o yadernyh reakciyah. Hotya yadernaya fizik imeet uzhe bol'shuyu istoriyu i mnozhestvo dostizhenii, tam ostaetsya mnogo voprosov. V pervuyu ochered' potomu, chto mnogie reakcii mozhno tol'ko rasschityvat' (t.e. net pryamyh izmerenii), a teoriya nepolna. I v astrofizike pri primenenii taih raschetov est' nekotoryi raznoboi: raznye gruppy ispol'zuyut raznye modeli i raschety. Avtory opisyvayut popytku kompilyacii raznyh dannyh v edinuyu biblioteku.
Authors: Elena Gallo, Don Marolf Comments: 15 pages, For the American Journal of Physics (15 pages). A Resource Letter is in large part an annotated bibliography. Comments and suggestions are welcome, though the goal is to keep the letter as brief as possible Poleznaya svodka literaturnyh istochnikov (ot populyarnyh knig do professional'nyh obzorov i original'nyh statei) po chernym dyram. V kakih-to aspektah, po vsei vidimosti, avtory idut na povodu lichnyh pristrastii (poskol'ku istochnikov velikoe mnozhestvo), gde-to mozhno bylo vklyuchit' bolee svezhie ssylki, tem ne menee ochen' poleznaya shtuka. Hotelos' by imet' takie po vsem vozmozhnym oblastyam :)
Authors: D.E. Winget, S.O. Kepler Comments: 70 pages, 11 figures, to be published in Annual Review of Astronomy and Astrophysics 2008 Bol'shoi obzor po pul'saciyam belyh karlikov. Poskol'ku obzor bol'shoi, to tam vsemu nashlos' mesto: i istoricheskomu vvedeniyu, i bazovomu opisaniyu fiziki belyh karlikov (zhurnal Annual Review of Astronomy and Astrophysics rasschitan skoree na nablyudatelei, chem teoretikov), i poyasneniyu togo zachem vse eto nuzhno (belye karliki - eto ochen' udobnye "relikty", po kotorym mozhno otslezhivat' raznye etapy evolyucii Galaktiki).
Authors: C.A.L. Bailer-Jones Comments: Proceedings of IAU 254 "The Galaxy disk in a cosmological context", Copenhagen, June 2008, invited talk, 8 pages Koroten'kii obzor, posvyashennyi budushemu astrometricheskomu sputniku Gaia i ozhidaemym rezul'tatam po svoistvam diska nashei Galaktiki. Yasno, chto poluchiv milliard tochnyh izmerenii polozhenii zvezd, sputnik sil'no prodvinet nashe ponimanie, tem ne menee interesno posmotret' detali.
Authors: Marco Taoso, Gianfranco Bertone, Georges Meynet, Sylvia Ekstrom Comments: 4 pages, 4 figures Zvezdy populyacii III obrazuyutsya iz veshestva nulevoi metallichnosti v galo temnoi materii na z~20. Razumeetsya, kakoe-to kolichestvo chastic temnogo veshestva okazyvaetsya vnutri zvezd. Eti chasticy mogut annigilirovat' drug s drugom, i lyudi davno zadumalis' nad vozmozhnymi posledstviyami. Na pal'cah posledstviya ochen' prosty. Vydelyaetsya dopolnitel'naya energiya, povyshaetsya temperatura. Zvezda (ili protozvezda) slegka rasshiryaetsya, chto ponizhaet temp yadernyh reakcii v zvezde, t.e. formirovanie zvezdy otkladyvaetsya ili zhe zvezda budet zhit' dol'she, poskol'ku medlennee rashoduet "goryuchee". Kachestvenno vse yasno, vopros s kolichestvennymi harakteristikami. Avtory ispol'zuyut odin iz luchshih v mire kodov po raschetu zvezdnoi evolyucii, chtoby posmotret' naskol'ko mozhno uvelichit' zhizn' zvezdy pri raznoi plotnosti temnogo veshestva. Imenno plotnost' chastic temnoi materii okazyvaetsya klyuchevym parametrom. Esli etih chastic nabrat' dostatochno mnogo, to - o chudo! - massivnaya pervozvezda mozhet voobshe dozhit' do nashih dnei. Odnako avtory ne issleduyut naskol'ko chasto takaya plotnost' budet nabirat'sya. Skoree vsego eto dostatochno redkaya situaciya. No kak bylo by interesno naiti ryadom massivnuyu zvezdu, obrazovavshuyusya, kogda eshe i galaktik-to nikakih ne bylo! Sm. takzhe stat'yu arxiv:0806.2662, gde avtory provodyat analogichnoe issledovanie i prihodyat k shozhim vyvodam.
Authors: O. Schnurr, A. F. J. Moffat, N. St-Louis, J. Casoli, A.-N. Chene Comments: 5 pages, 4 figures; accepted for MNRAS Letters V stat'e rasskazyvaetsya ob obnaruzhenii dvoinoi, sostoyashei iz dvuh ochen' massivnyh zvezd. Esli ocenki massy verny, to eto prosto samaya massivnaya dvoinaya: 116 (+/-31) i 89 (+/-16) mass Solnca. Prichem, bolee massivnyi komponent pary pretenduet na zvanie samoi massivnoi zvezdy.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: E.A. Baltz et al. Comments: 49 pages, 29 figures, JCAP in press Avtory delayut detal'nye ocenki togo, kak GLAST mozhet registrirovat' temnuyu materiyu po annigilyacionnomu signalu. Chasticy temnoi materii mogut annigilirovat' drug s drugom. Sootvetstvenno, "v mestah massovogo skopleniya" etih chastic mozhno ozhidat' sil'nogo gamma-izlucheniya, popadayushego v diapazon chuvstvitel'nosti GLAST. V pervuyu ochered' rech' idet o central'noi chasti nashei Galaktiki. V stat'e ochen' podrobno razobrano chto i kak budet registrirovat' pribor LAT. Ozhidaniya ochen' ser'eznye.
Authors: G.A. Tammann, A. Sandage, B. Reindl Comments: 44 pages, 4 figures, 6 tables, accepted for publication in the Astronony and Astrophysics Review 159 Tammann i Sendedzh - izvestneishie specialisty v oblasti opredeleniya rasstoyanii do galaktik i, sootvetstvenno, dinamiki rasshireniya vselennoi. V etoi stat'e privodyatsya dannye po 279 galaktikam na rasstoyaniyah do 2000 km/s, dlya kotoryh polucheny dostatochno tochnye nezavisimye ocenki rasstoyanii po cefeidam, sverhnovym Ia i krasnym gigantam. Dopolnitel'no obsuzhdayutsya eshe 62 bolee dalekie galaktiki (do 20 000 km/s), dlya kotoryh rasstoyaniya polucheny po sverhnovym Ia. Opredeleno znachenie postoyannoi Habbla 60-65 km/s/Mpk.
Authors: Michael W. Feast Comments: 5 pages, For Proc. Middle-East Africa Regional IAU Meeting, Cairo 2008 Daetsya kratkaya svodka sostoyaniya del v opredelenii rasstoyanii po razlichnym tipam peremennyh zvezd (razlichnye cefeidy i rodstvennye im zvezdy, miridy). Takzhe privodyatsya ocenki rasstoyaniya do centra Galaktiki i postoyannaya Habbla, poluchennye v ramkah proekta.
Authors: Keivan G. Stassun et al. Comments: 23 pages, Published in Nature, 19 June 2008 Avtory issleduyut paru molodyh zvezd. Massa komponent dvoinoi identichna s tochnost'yu okolo 2 procentov (0.4 massy Solnca). A vot temperatury, radiusy i svetimosti razlichayutsya gorazdo sil'nee. Avtory polagayut, chto edinstvennym razumnym ob'yasneniem yavlyaetsya raznyi vozrast dvuh komponentov dvoinoi. Vot takoi vot "paradoks bliznecov". Situaciya udivitel'na. Obychno polagayut, chto vozrast zvezd v dvoinoi sisteme odinakov (osobennoe, kogda massy primerno ravny). Eto predpolozhenie dazhe ispol'zuetsya pri kalibrovkah-normirovkah. A tut takoe otkrytie! Sistema yavlyaetsya zatmennoi dvoinoi. Vozrast okolo milliona let (eto samaya molodaya zatmennaya sistema so zvezdami-bliznecami). Nablyudeniya spektrov vysokogo razresheniya byli provedeny na teleskope Hobbi-Eberli.
Obsudit' v ZhZh-soobshestve
ru_astroph
Authors: Neil M. Nagar, Javier Matulich Comments: 9 pages total. To appear in A&A Avtory pishut, chto dlya 27 chastic s energiyami vyshe 56 EeV naibolee veroyatnymi mestami rozhdeniya yavlyayutsya blizkie radiogalaktiki. Pri etom galaktik po morfologii i tp. ne ochen' pohozhi na M87 (otsutstvie sushestvennogo potoka ot M87 mnogimi rassmatrivaetsya kak argument protiv svyazi etih chastic s blizkimi aktivnymi galaktikami). Sushestvenno, chto rech' ne o vseh zaregistrirovannyh chasticah so stol' vysokoi energiei, a o podvyborke. Net somnenii, chto rabotu eshe budut kritikovat', i diskussiya prodolzhitsya.
Authors: Steven B. Giddings, Michelangelo M. Mangano Comments: 97 pages Avtory rassmatrivayut samye raznoobraznye varianty, svyazannye s sushestvovaniem TeVnyh chernyh dyr (takie, naprimer, mogut proizvodit'sya na uskoritele LHC), esli oni ustoichivy. V chastnosti, avtory rassmatrivayut v ramkah razlichnyh scenariev, kak tikaie chernye dyry budut akkrecirovat', nahodyas' v Zemle. rezyume dovol'no optimistichnoe. Takzhe rassmatrivayutsya takie chernye dyry, rozhdennye v kosmicheskih luchah, i mnogoe-mnogoe drugoe. V stat'e vse-taki 97 stranic!!!
Obsudit' v ZhZh-soobshestve
ru_astroph.
My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing).
Authors: Zita Martins et al. Comments: 31 pages, 4 figures, 3 tables Journal-ref: Earth and Planetary Science Letters 270, 130-136. 15 June 2008 Nashumevshaya stat'ya ob obnaruzhenii v meteorite slozhnyh organicheskih soedinenii yakoby vnezemnogo proishozhdeniya.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: Borexino Collaboration: G. Alimonti, et al Comments: 37 pages, 43 figures, to be submitted to NIM Podrobno opisyvaetsya neitrinnyi detektor Boreksino.
Authors: Makoto Tsubota Comments: 13 pages, 5 figures, Review article to appear in J. Phys. Soc. Jpn Sushestvuet takoe lyubopytneishee yavlenie, otkrytoe eshe v 50-e gg. v zhidkom gelii-4. Seichas ono avtivno izuchaetsya i eksperimentatorami, i teoretikami.
Authors: S. Scorza Comments: 4 pages, 43rd Rencontres de Moriond - Electroweak Interactions and Unified Theories, La Thuile : Italie (2008) Kratko opisan eksperiment EDELWEISS-II. On prednaznachen dlya laboratornyh poiskov chastic temnoi materii. V 2006-2007 gg. provodilis' tehnologicheskie progony. V etom planiruetsya pervaya seriya nauchnyh nablyudenii.
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