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The R.A.P.Project "Prosto o slozhnom" "Astro-ph za 2006 g." Nemnogo statistiki Predydushii vypusk (N159) Slovar' astroterminov Spisok missii i teleskopov Obzory UFN Stat'i SOZh ANKa Dnya 14.03.2007. Taina kolec sverhnovoi 06.03.2007. BL Lac v zhestkom gamma 21.09.2006. Vspyshka vnegalakticheskogo magnitara ili korotkii gamma-vsplesk? 23.08.2006. Chernaya koshka obnaruzhena 13.04.2006. On bol'she Plutona! 07.04.2006. Disk vokrug anomal'nogo pul'sara 29.03.2006. Samyi dalekii gamma-vsplesk: mesto rozhdeniya 22.03.2006. Vega krutitsya volchkom 21.03.2006. Tri goda raboty WMAP 03.03.2006. S chem mozhno pereputat' sverhnovuyu? Soderzhanie i bystryi perehod k razdelam obzora Stat'i nedeli "Luchshie iz luchshih" arxiv/0706.0123 Astrofizika rannego obrazovaniya galaktik arxiv/0706.0500 Bolee glubokii poisk praroditelya sverhnovoi tipa Ic 2002ap arxiv/0706.0516 Kinematika ul'traslabyh sputnikov Galaktiki: reshenie problemy nedostayushih sputnikov arxiv/0706.0867 Izobrazhenie poverhnosti Al'taira arxiv/0706.0914 Chetyre kvazara na krasnyh smesheniyah bol'she 6, otkrytye v kanadsko-francuzskom obzore kvazarov na vysokih krasnyh smesheniyah Otdel'nye stat'i Astrofizika rannego obrazovaniya galaktik Pervobytnye galaktiki Bolee glubokii poisk praroditelya sverhnovoi tipa Ic 2002ap Kinematika ul'traslabyh sputnikov Galaktiki: reshenie problemy nedostayushih sputnikov LISA: Mars i predely dlya zhizni Kerrovskoe prostranstvo-vremya: kratkoe vvedenie Izobrazhenie poverhnosti Al'taira Ogranichenie na kiki belyh karlikov v sharovyh skopleniyah Ul'tramoshnyi rentgenovskii istochnik vblizi centra M82 Chetyre kvazara na krasnyh smesheniyah bol'she 6, otkrytye v kanadsko-francuzskom obzore kvazarov na vysokih krasnyh smesheniyah Kompaktnyi rentgenovskii istochnik 1E 1547.0-5408 v radioobolochke G327.24-0.13: novyi vozmozhnyi primer associacii mezhdu kandidatom v magnitary i kandidatom v ostatki sverhnovyh Iz razdela physics Bol'cman i iskusstvo poleta 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 (36.9 Mb; *.tar.gz) gzip homepage Razdely arhiva (s aprelya 2003 g.): kosmologiya, neitrino, kosmicheskie luchi i gamma-astronomiya, galaktiki, AYaG, kvazary, nasha Galaktika, mezhzvezdnaya sreda, zvezdy, sverhnovye, ostatki sverhnovyh, chernye dyry, neitronnye zvezdy, linzirovanie, Solnce, ekzoplanety, Solnechnaya sistema, akkreciya, tesnye dvoinye sistemy, gamma-vspleski, gravitacionnye volny, mehanizmy izlucheniya, chislennoe modelirovanie, dinamika, mehanika metody obrabotki dannyh, MGD, metody nablyudenii, budushie nablyudatel'nye proekty, prochee. Poleznye astronomicheskie ssylki. Korotkoe esse ob elektronnyh preprintah. Obzornye stat'i v astro-ph 2001-2003 gg. Obsudit' na forume Scientific.RU Obsudit' na forume Zvezdocheta Avtor proekta Sergei Popov Diskussii po stat'yam Arhiva PhysComments CosmoCoffee Postav'te u sebya nashu knopku! Proekt razmeshen na saitah: Smotri takzhe diskussii i blogi: Informacionnye partnery Vy mozhet takzhe razmestit' na svoem saite nashu lentu obzorov Kniga avtora obzorov Novostnye lenty 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 N160 astro-ph za 01 - 08 iyunya 2007 goda: izbrannye stat'i Referaty otdel'nyh statei obzor arxiv:0706.0123 Astrofizika rannego obrazovaniya galaktik (The Astrophysics of Early Galaxy Formation) Authors: Piero Madau Comments: 39 pages, to appear in the proceedings of the XVIII Canary Islands Winter School of Astrophysics on "The Emission Line Universe", J. Cepa and F. Sanchez eds., Cambridge University Press V lekcii sobrano bolee-menee vse, chto nuzhno znat' dlya pervogo (no ser'eznogo) znakomstva s formirovaniem krupnomasshtabnoi struktury, formirovaniem i evolyuciei galaktik i pervymi zvezdami. V obzore mnogo poleznyh formul i zavisimostei. V obshem, vse ochen' ser'ezno, dostatochno polno i po delu. Horoshim dopolneniem posluzhit sleduyushii punkt nashei programmy. obzor arxiv:0706.0139 Pervobytnye galaktiki (Primeval galaxies) Authors: Daniel Schaerer Comments: 48 pages including figures. Lecture notes to appear in "The emission line Universe", XVIII Canary Islands Winter School of Astrophysics, Ed. J. Cepa, Cambridge Univ. Press Eti lekcii posvyasheny pervym galaktikam i zvezdam. Zdes' formul uzhe prakticheski net, zato est' mnogo nablyutel'nyh dannyh i rezul'tatov sravneniya model'nyh raschetov s nablyudeniyami. Tak chto material v samom dele prekrasno dopolnyaet predydushii. arxiv:0706.0500 Bolee glubokii poisk praroditelya sverhnovoi tipa Ic 2002ap (A deeper search for the progenitor of the Type Ic Supernova 2002ap) Authors: R. M. Crockett, et al. Comments: 20 pages, 11 figures (resolution of images reduced), 6 tables, submitted for publication in MNRAS Izuchenie sverhnovyh vyshlo na novyi uroven', kogda stalo vozmozhnym iskat' zvezdy-praroditeli na arhivnyh snimkah. Pravda, primery, kogda praroditel' byl identificirovan, mozhno pereschitat' po pal'cam. V obsuzhdaemoi stat'e praroditel' ne naiden, no postavleny ochen' vazhnye verhnie predely, krome togo, rech' idet o sverhnovyh tipa Ic. Verhnii predel govorit o tom, chto praroditelem mogla byt' tol'ko zvezda Vol'fa-Raie. Prichem, esli eto byla odinochnaya zvezda, to ona dolzhna byla by imet' ochen' bol'shoi temp poteri massy, bol'she standartnogo. Znachit, veroyatnee vsego, zvezda-praroditel' vhodila v dvoinuyu sistemu. Sootvetstvenno, mozhno posmotret' ne viden li seichas vtoroi komponent. Ne viden. Znachit, mozhno dat' ogranichenie na ego massu, esli eto normal'naya zvezda (razumeetsya, kompan'on mozhet byt' kompaktnym ob'ektom). V obshem, na moi vzglyad, nablyudeniya nachinayut davat' ochen' vazhnye dlya modelei sverhnovyh dannye. arxiv:0706.0516 Kinematika ul'traslabyh sputnikov Galaktiki: reshenie problemy nedostayushih sputnikov (The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem) Authors: Joshua D. Simon, Marla Geha Comments: 21 pages, 15 figures (12 in color), 6 tables. Submitted to ApJ Kak izvestno, sushestvuet t.n. "problema nedostayushih sputnikov". Chislennoe modelirovanie formirovaniya galaktik v modeli ierarhicheskogo skuchivaniya predskazyvaet, chto u nashei Galaktiki dolzhno byt' gorazdo bol'she slabyh sputnikov, chem nablyudaetsya. Problema dovol'no ser'eznaya, i aktivno obsuzhdaetsya. Takzhe izvestno, chto v poslednee vremya (vo mnogom blagodarya Sloanovskomu obzoru - SDSS) otkryvayut mnogo karlikovyh galaktikov - sputnikov Mlechnogo Puti. Avtory detal'no issleduyut vosem' nedavno otkrytyh sputnikov i pytayutsya ponyat', mozhno li tut kak-to reshit' problemu nehvatki karlikovyh galaktik. Razumeetsya, novye otkrytiya sushestvenno smyagchayut problemu, no ne reshayut ee polnost'yu Sputnikov vse ravno ne hvataet, i nuzhny dopolnitel'nye predpolozheniya. Avtory pokazyvayut, chto naibolee effektivnoi budet gipoteza o tom, chto lish' dostatochno massivnye galo temnoi materii (a vse galaktiki, vklyuchaya i karlikovye sputniki, eto v osnovnom temnaya materiya, v ne obychnoe veshestvo) sposobny formirovt' zvezdy. Prichem, nabrat' etu kriticheskuyu massu nado bylo do epohi reionizacii. Esli eto udaetsya, to v nastoyashii moment my uvidim takoi ob'ekt kak galaktiku, esli zhe net, to budet lish' temnoe galo, uskol'zayushee ot nashih nablyudenii. arxiv:0706.0530 LISA: Mars i predely dlya zhizni (LISA: Mars and the limits of life) Authors: G. Galletta, et al. Comments: 4 pages, 3 figures. Mem. SAIt, in press LISA - Laboratorio Italiano di Simulazione Ambiente (Ital'yanskaya laboratoriya dlya modelirovaniya okruzhayushei sredy, sm. opisanie proekta na ital'yanskom yazyke). Proekt realizovan v Padue. Eksperiment pozvolyaet modelirovat' usloviya ot normal'nyh dlya cheloveka do marsianskih. Imenno marsianskoi chasti proekta i posvyashena korotkaya zametka. Bylo provedeno neskol'ko "progonov", v kotoryh spory i bakterii podvergalis' "vnezemnym" mucheniyam v usloviyah, pohozhih na marsianskie. Cel'yu bylo proverit' vyzhivut ili net. Koe-kakie obrazcy vyzhivali. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. obzor arxiv:0706.0622 Kerrovskoe prostranstvo-vremya: kratkoe vvedenie (The Kerr spacetime: A brief introduction) Authors: Matt Visser Comments: 37 pages, 1 figure: This is a draft of an introductory chapter on the Kerr spacetime that is intended for use in the book "The Kerr spacetime", currently being edited by Susan Scott, Matt Visser, and David Wiltshire. Na samom dele, ne takoe uzh kratkoe, i sovsem ne prostoe vvedenie v kerrovskuyu metriku. Hotya prostota sostoit, pozhalui, v tom, chto vypisany mnogie formuly, bez kotoryh potom sovsem nel'zya vlezat' v detali (detali - v knige, mozhet byt' i ona poyavitsya v svoe vremya v seti). arxiv:0706.0867 Izobrazhenie poverhnosti Al'taira (Imaging the Surface of Altair) Authors: John D. Monnnier et al. Comments: 24 pages. to appear in Science. includes Report and Supplemental Online Materials. Accompanying animation can be found at this http URL Vot i poyavilsya polnyi tekst raboty, o kotoroi tak mnogo pisali v SMI. S pomosh'yu interferometra, rabotayushego v blizhnem IK diapazone, udalos' poluchit' neplohie izobrazheniya al'fa Orla. Uglovoe razreshenie luchshe odnoi tysyachnoi sekundy dugi (v itoge chto-to okolo odnoi desyatimillionnoi gradusa, ili, esli ugodno, odnoi milliardnoi dugi, nemnogo okruglyaya). Razumeetsya, dlya ob'yasneniya bolee detal'nyh dannyh nuzhny i bolee detal'nye zvezdnye modeli. Teoretiki berutsya za rabotu. arxiv:0706.0900 Ogranichenie na kiki belyh karlikov v sharovyh skopleniyah (Constraining white-dwarf kicks in globular clusters) Authors: Jeremy S. Heyl Comments: 4 pages, 3 figures, submitted to MNRAS Letters Na stadii asimptoticheskoi vetvi gigantov zvezdnyi veter mozhet byt' sil'nym i sushestvenno asimmetrichnym. Itogo mozhet stat' razgon ostayushegosya zvezdnogo yadra - budushego belogo karlika. V nekotorom smysle mozhno skazat', chto kak i neitronnye zvezdy, belye karliki pri svoem rozhdenii poluchayut kik (kick - udar, tolchok). Konechno, sbros obolochki gigantom - eto ne vzryv sverhnovyh, poetomu kik u belyh karlikov ne mozhet dostigat' tysyach km/s, kak u neitronnyh zvezd. Tem ne menee, mogut byt' nablyudatel'nye effekty, svyazannye s raspredeleniem belyh karlikov v sharovyh skopleniyah. Vo-pervyh, chast' belyh karlikov mozhet prosto vyletat' iz skoplenii, t.e. budet nablyudat'sya ih deficit. Vo-vtoryh, molodye karliki (kotorye eshe ne uspeli vyletet') budut menee koncentrirovany k centru skopleniya. Poslednee - nablyudaetsya. T.o., polagaet Dzheremi Heil, raspredelenie molodyh belyh karlikov v sharovyh skopleniyah mozhet posluzhit' unikal'nym instrumentom dlya izucheniya poteri massy na asimptoticheskoi vetvi gigantov i vo vremya formirovaniya planetarnyh tumannostei. Sm. takzhe arxiv:0706.0912. V etoi stat'e Heil rassmatrivaet vozdeistvie kika belyh karlikov na ih zhizn' v tesnoi dvoinoi sisteme. arxiv:0706.0901 Ul'tramoshnyi rentgenovskii istochnik vblizi centra M82 (The Ultraluminous X-ray Sources near the Center of M82) Authors: A.K.H. Kong et al. Comments: 10 pages, 8 figures. Submitted to ApJ Po dannym nablyudenii na Chandre v central'noi oblasti izvestnoi blizkoi galaktiki s moshnym zvezdoobrazovaniem M82 otkryt tranzientnyi ul'tramoshnyi istochnik (audiofail s zapis'yu nauchno-populyarnoi programmy, v kotoroi shla rech' ob etih ob'ektah, mozhno naiti zdes'). Raspolozhen ob'ekt v molodom zvezdnom skoplenii. Avtory polagayut, chto my imeem delo s chernoi dyroi promezhutochnoi massy (bolee 100 solnechnyh). arxiv:0706.0914 Chetyre kvazara na krasnyh smesheniyah bol'she 6, otkrytye v kanadsko-francuzskom obzore kvazarov na vysokih krasnyh smesheniyah (Four quasars above redshift 6 discovered by the Canada-France High-z Quasar Survey) Authors: Chris J. Willott, et al. Comments: 14 pages, 9 figures, submitted to AJ Predstavleny svezheotkrytye dalekie kvazary. Sredi nih - samyi dalekii na segodnyashnii den': CFHQS J2329-0301. On nahoditsya na krasnom smeshenii z=6.43 (napomnyu, chto perevod krasnyh smeshenii v rasstoyaniya ili vremya ot bol'shogo vzryva yavlyaetsya model'no zavisimoi proceduroi). Sm. takzhe novost' na Granyah. arxiv:0706.1054 Kompaktnyi rentgenovskii istochnik 1E 1547.0-5408 v radioobolochke G327.24-0.13: novyi vozmozhnyi primer associacii mezhdu kandidatom v magnitary i kandidatom v ostatki sverhnovyh (The Compact X-ray Source 1E 1547.0-5408 and the Radio Shell G327.24-0.13: A New Proposed Association between a Candidate Magnetar and a Candidate Supernova Remnant) Authors: Joseph D. Gelfand, B. M. Gaensler Comments: 11 pages, 5 figures, ApJ accepted Avtory predstavlyayut rezul'taty nablyudenii v raznyh diapazonah istochnika 1E 1547.0-5408. Po mneniyu avtorov, my imeem delo s magnitarom, k tomu zhe, vo vsei vidimosti, nahodyashimsya v ostatke sverhnovoi. Tak eto ili net na samom dele pokazhut dal'neishie issledovaniya. My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing). arxiv:0706.0008 Bol'cman i iskusstvo poleta (Boltzmann and the art of flying) Authors: Silvio R. Dahmen Comments: 15 pages, no figures Pochemu lyudi ne letayut kak pticy Posle nebol'shogo razbega avtor rasskazyvaet ob entuziazme Bol'cmana v oblasti vozduhoplavaniya. Opisyvayutsya lekcii Bol'cmana, posyashennye dannoi probleme, ego lichnye kontakty i, v chastnosti, perepiska s entuziastami poletov na apparatah tyazhelee vozduha. Vernut'sya k nachalu stranicy

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