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The R.A.P.Project "Prosto o slozhnom" "Astro-ph za 2006 g." Nemnogo statistiki Predydushii vypusk (N193) Slovar' astroterminov Spisok missii i teleskopov Obzory UFN Stat'i SOZh ANKa Dnya 09.09.2008. Chernyi val's s feierverkom 29.08.2008. "Kotik, cheshirchik ...." 28.08.2008. Ne temnaya li eto materiya nasledila? 19.08.2008. Ochen' legkii millisekundnyi pul'sar 08.08.2008. Portret beta Liry 22.01.2008. Chernaya dyra v Omega Centavra 11.01.2008. Dvoinoe einshteinovskoe kol'co 06.08.2007. Kto eto tam tak bumknul? 14.03.2007. Taina kolec sverhnovoi 06.03.2007. BL Lac v zhestkom gamma Soderzhanie i bystryi perehod k razdelam obzora Stat'i nedeli "Luchshie iz luchshih" arxiv/0809.0510 Novyi klass moshnyh tranzientov i pervaya peprepis' ih massivnyh praroditelei arxiv/0809.0631 Pervichnyi nukleosintez: ot tochnoi kosmologii k fundamental'noi fizike arxiv/0809.1280 Massivnaya dvoinaya iz dvuh chernyh dyr v OJ287 i testy obshei teorii otnositel'nosti arxiv/0809.1648 Otkrytie neobychnogo opticheskogo tranzienta s pomosh'yu Kosmicheskogo teleskopa imeni Habbla Otdel'nye stat'i Obzory galaktik na bol'shih krasnyh smesheniyah Chto zhe Habbl deistvitel'no imel vvidu pod rannimi i pozdnimi tipami: prosto bolee ili menee slozhnuyu vidimuyu strukturu VLT zaregistriroval krasnyi gigant - praroditelya sverhnovoi 2008bk, imevshei tip IIP Ispol'zovanie kosmicheskogo teleskopa SPICA dlya issledovanie ekzoplanet Blizhaishaya OV associaciya: Skorpion-Centavr (Sco OB2) Novyi klass moshnyh tranzientov i pervaya peprepis' ih massivnyh praroditelei Obrazovanie i evolyuciya diskovyh galaktik Pervichnyi nukleosintez: ot tochnoi kosmologii k fundamental'noi fizike Gravitacionno-volnovoi signal ot sverhnovyh s kollapsom yadra Shema dlya registracii supersimmetrichnoi temnoi materii v galo Galaktiki Istochniki INTEGRAL: ot massivnyh rentgenovskih dvoinyh s sil'nym poglosheniem k bystrym rentgenovskim tranzientam so sverhgigantami Katalog tochechnyh rentgenovskih istochnikov po dannym dvuhmegasekundnyh nablyudenii galakticheskogo centra na Chandre Registraciya zaderzhannogo gamma-izlucheniya ot GRB 080514B na AGILE Massivnaya dvoinaya iz dvuh chernyh dyr v OJ287 i testy obshei teorii otnositel'nosti Gravitacionno-volnovaya astronomiya Otkrytie neobychnogo opticheskogo tranzienta s pomosh'yu Kosmicheskogo teleskopa imeni Habbla Udarnaya volna ot vzryva Eta Kilya 1843 goda Obrazovanie i evolyuciya kataklizmicheskih peremennyh Iz razdela physics Lord Rezerford, ego nobelevskaya premiya 1908 goda po himii, i pochemu on ne poluchil vtoruyu premiyu 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 Obsudit' v bloge na Subscribe.ru Avtor proekta Sergei Popov Ranee uchastvovali: Mihail Prohorov Ekaterina Kasimova Diskussii po stat'yam Arhiva CosmoCoffee arXiv Blog 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 N194 astro-ph za 01 - 11 sentyabrya 2008 goda: izbrannye stat'i Referaty otdel'nyh statei miniobzor arxiv:0809.0050 Obzory galaktik na bol'shih krasnyh smesheniyah (High redshift galaxy surveys) Authors: Masanori Iye Comments: Plenary talk given on 25 June at the SPIE 2008 symposium on "Astronomical Instrumentation" in Marseiile, 10 pages, SPIE Proc. 7016, 701602, (2008) Nebol'shoi, no soderzhatel'nyi obzor s bol'shim chislom ssylok, posvyashennyi razlichnym metodam poiska i nablyudenii galaktik na bol'shih krasnyh smesheniyah. Metody vklyuchayut v sebya poisk laiman-al'fa-emitterov, poisk po laimanovskomu zavalu, issledovanie gravitacionnyh linz, issledovaniya kvazarov i hozyaiskih galaktik gamma-vspleskov. arxiv:0809.0125 Chto zhe Habbl deistvitel'no imel vvidu pod rannimi i pozdnimi tipami: prosto bolee ili menee slozhnuyu vidimuyu strukturu (What Hubble really meant by late and early type: simply more or less complex in appearance) Authors: I. K. Baldry Comments: 3 pages, 2 figures, using MNRAS style file; to appear in RAS journal Astronomy & Geophysics (A&G), scheduled for October 2008 issue Lyubopytnaya korotkaya zametka. Vse znayut kamerton Habbla. Dostatochno chasto mozhno prochest', chto Habbl podrazumeval eto kak evolyucionnuyu posledovatel'nost' ot galaktik rannih tipov (ellipticheskih) k pozdnim. Avtor pokazyvaet, chto eto ne tak. Tochno takzhe kak rannie i pozdnie tipy zvezdnyh spektrov otrazhayut lish' ih menee (rannie) ili bolee (pozdnie) strukturu, tak zhe i klassifikaciya galaktik ne podrazumevaet posledovatel'nosti vo vremeni, a lish' govorit o vneshnem vide. Hotya Habbl i pishet, chto podrazumevanie vremennoi posledovatel'nosti na sovesti avtora. Obsudit' v ZhZh-soobshestve ru_astroph Obsudit' na Astroforume v Nauchnoi panorame. arxiv:0809.0206 VLT zaregistriroval krasnyi gigant - praroditelya sverhnovoi 2008bk, imevshei tip IIP (VLT detection of a red supergiant progenitor of the type IIP supernova 2008bk) Authors: S. Mattila, S.J. Smartt, J.J. Eldridge, J.R. Maund, R.M. Crockett, I.J. Danziger Comments: 4 pages, 2 figures, submitted to ApJ letters Na snimkah, sdelannyh VLT, udalos' rassmotret' zvezdu-praroditelya sverhnovoi 2008bk. Sverhnovaya imela tip IIP. Izuchenie praroditelya pokazalo, chto on imel nachal'nuyu massu ot 7.5 do 9.5 mass Solnca. Drugaya interesnaya rabota po praroditelyam sverhnovyh - arxiv:0809.0236. V nei avtory issleduyut raspredelenie sverhnovyh v galaktikah, sravnivaya ego s polozheniem oblastei zvezdoobrazovaniya. Sverhnovye tipa II huzhe vsego otslezhivayut zvezdoobrazovaniya. Tipa Ic - luchshe vsego. Iz etogo avtory delayut vyvod, chto posledovatel'nost' II-Ib-Ic otrazhaet rost massy zvezd-praroditelei. Eshe odna stat'ya arxiv:0809.0403 posvyashena nablyudatel'nym ogranicheniyam na praroditelei SN IIP. Minimal'naya massa praroditelei etih sverhnovyh 7-9.5 mass Solnca. arxiv:0809.0242 Ispol'zovanie kosmicheskogo teleskopa SPICA dlya issledovanie ekzoplanet (Using SPICA Space Telescope to characterize Exoplanets) Authors: J.R. Goicoechea et al. Comments: 11 pages, White Paper for ESA's Exo-Planet Roadmap Advisory Team, submitted on 2008 July 29 Opisan proekt SPICA, predlozhennyi sovmestno evropeiskim i yaponskim kosmicheskimi agentstvami. Eto orbital'nyi 3.5-metrovyi infrakrasnyi teleskop. Odna iz zadach - issledovaniya ekzoplanet. V stat'e v osnovnom ob etom i idet rech'. Proekt poka na stadii rassmotreniya v ramkah programmy ESA Cosmic Vision 2015-2025. obzor arxiv:0809.0407 Blizhaishaya OV associaciya: Skorpion-Centavr (Sco OB2) (The Nearest OB Association: Scorpius-Centaurus (Sco OB2)) Authors: Thomas Preibisch, Eric Mamajek Comments: 50 pages, Chapter for the "Handbook of Star Forming Regions", Vol. II: The Southern Sky, Bo Reipurth, ed Svedeny voedino vse dannye po samoi blizkoi k nam associacii Sco OB2. Razumeetsya, poskol'ku rech' idet o blizhaishei associacii, to ona ispol'zuetsya kak nekotoryi poligon dlya izucheniya podobnyh obrazovanii. Ona sostoit iz treh grupp raznyh vozrastov (5, 16 i 17 millionov let). Blagodarya blizosti mozhno izuchat' ne tol'ko massivnye zvezdy. arxiv:0809.0510 Novyi klass moshnyh tranzientov i pervaya peprepis' ih massivnyh praroditelei (A New Class of Luminous Transients and A First Census of Their Massive Stellar Progenitors) Authors: Todd A. Thompson et al. Comments: 21 pages, emulateapj, 11 figures, 3 tables; submitted to ApJ Nedavno bylo obnaruzheno dva sobytiya, kotorye po vsei vidimosti yavlyayutsya sverhnovymi, no ih zvezdna velichina byla neskol'ko men'she. Opredeleny zvezdy-praroditeli etih vzryvov. Avtory polagayut, chto vo-pervyh, eti sobytiya formiruyut novyi tip zvezdnyh vzryvov, sostavlyayushii kak minimum bolee 10 procentov ot vseh sverhnovyh, svyazannyh s kollapsom yadra. Vo-vtoryh, oni delayut eshe bolee interesnyi vyvod. Delo v tom, chto vokrug zvezd-praroditelei etih vzryvov ochen' mnogo pyli. My znaem takie zvezdy, no ih ochen' malo. T.e., esli prosto vzorvat' izvestnye stol' zapylennye zvezdy, to temp vzryvov budet slishkom nizkim. Otsyuda avtory delayut sleduyushii vyvod. Za neskol'ko tysyach let do vzryva mnogoe massivnye zvezdy (mnogie, no ne vse, dazhe, vidimo, men'shinstvo, no vse ravno rech' idet kak minimum o desyati procentah, a skoree neskol'ko bol'she) obrazuyut vokrug sebya mnogo-mnogo pyli. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. miniobzor arxiv:0809.0513 Obrazovanie i evolyuciya diskovyh galaktik (Formation and evolution of disk galaxies) Authors: Joseph Silk Comments: 9 pages, to appear in The Galaxy Disk in Cosmological Context Proceedings IAU Symposium No. 254, 2008, J. Andersen, J. Bland-Hawthorn & B. Nordstrm, eds Nebol'shoi obzor, v kotorom obsuzhdaetsya, kak nahodyat svoe ob'yasneniya nekotorye bazovye fenomenologicheskie sootnosheniya (naprimer, Talli-Fishera). Obzor interesen naborom prostyh formul i poyasnenii, kotorye pokazyvayut, kak v dovol'no prostyh modelyah mozhno opisat' osnovnye etapy evolyucii diskovyh galaktik. megaobzor arxiv:0809.0631 Pervichnyi nukleosintez: ot tochnoi kosmologii k fundamental'noi fizike (Primordial Nucleosynthesis: from precision cosmology to fundamental physics) Authors: F. Iocco, G. Mangano, G. Miele, O. Pisanti, P.D. Serpico Comments: 147 pages, 69 figures, submitted to Physics Reports Vse, chto vy hoteli znat' o pervichnom nukleosinteze. Plyus obzor osnov po kosmologii. Napomnyu, chto pervichnyi nukleosintez - eto odna iz chetyreh kolonn, na kotoryh stoit sovremennaya kosmologiya. obzor arxiv:0809.0695 Gravitacionno-volnovoi signal ot sverhnovyh s kollapsom yadra (The Gravitational Wave Signature of Core-Collapse Supernovae) Authors: Christian D. Ott Comments: Topical Review, submitted to CQG. 49 pages, 13 figures Bol'shoi obzor po ozhidaemym gravitacionno-volnovym signalam ot sverhnovyh, svyazannyh so vzryvami massivnyh zvezd. arxiv:0809.0894 Shema dlya registracii supersimmetrichnoi temnoi materii v galo Galaktiki (A blueprint for detecting supersymmetric dark matter in the Galactic halo) Authors: Volker Springel et al. Comments: to appear in Nature, 23 pages, 8 figures, includes Supplementary Information V svyazi s nachalom uspeshnoi raboty Fermi-GLAST aktivizirovalas' aktivnost', svyazannaya s raschetami registriruemosti gamma-luchei ot temnoi materii v nashei Galaktike. Poyavilos' srazu neskol'ko rabot. Shpringel i soavtory v svoei stat'e v Nature rassmatrivayut sleduyushuyu problemu. Izvestno, chto temnoe veshestvo raspredeleno v galo neravnomerno. Vo-pervyh, est' sobstvenno galo nashei Galaktiki, vo-vtoryh v nem est' subgalo (ih chislo ochen' veliko - poryadka 100 000), v-tret'ih, i v galo i v subgalo est' struktury. Sprashivaetsya, signal ot kakih obrazovanii budet zametnee? Shpringel i soavtory reshayut etu problemu s pomosh'yu detal'nogo chislennogo modelirovaniya (bolee podrobno sm. arxiv:0809.0898). Otvet, davaemyi v stat'e, takov. Zametnee budet signal ot osnovnogo galo. Razumeetsya, on sil'nee iz central'noi chasti Galaktiki (polovina signala ot vsego galo idet iz oblasti s radiusom primerno 2.6 kpk). Hotya subgalo summarno i dominiruyut v polnoi svetimosti (esli smotret' na nashu Galaktiku izdaleka, to osnovnoi annigilyacionnyi signal budet svyazan s subgalo), no dlya nablyudatelya na Zemle subgalo - dostatochno dalekie istochniki. Poetomu my zhdem signala v pervuyu ochered' iz central'noi chasti Mlechnogo Puti. Eshe v odnoi stat'e (arxiv:0809.0901) takzhe s pomosh'yu chislennogo modelirovaniya issleduetsya struktura i obrazovaniya galo temnoi materii. A v arxiv:0809.0886 obsuzhdaetsya, smozhet li Fermi-GLAST obnaruzhit' sobstvennoe dvizhenie subgalo. Otvet: skoree vsego net, t.k. maloveroyatno, chto dazhe blizhaishee k nam subgalo budet dostatochno blizko dlya etogo. Takzhe vopros o vozmozhnoi registracii temnoi materii putem nablyudeniya gamma-izlucheniya ot annigilyacii i svoistva galo obsuzhdayutsya v arxiv:0809.1523. obzor arxiv:0809.1076 Istochniki INTEGRAL: ot massivnyh rentgenovskih dvoinyh s sil'nym poglosheniem k bystrym rentgenovskim tranzientam so sverhgigantami (INTEGRAL sources: from obscured high mass X-ray binaries to supergiant fast X-ray transients) Authors: S. Chaty Comments: Lecture given in the First La Plata International School on Astronomy and Geophysics: Compact Objects and their emission, La Plata Observatory, 10-14 March 2008, Argentina, 20 pages, 2 figures, 1 table, editors P. Benaglia and G. Romero Sputnik INTEGRAL, blagodarya vysokoi chuvstvitel'nosti v ochen' zhestkom rentgenovskom diapazone i dlitel'nym nablyudeniyam ploskosti Galaktiki, smog obnaruzhit' mnogo novyh interesnyh istochnikov, svyazannyh s tesnymi dvoinymim sistemami. Obnaruzheno dva novyh klassa istochnikov. Vo-pervyh, eto bystrye rentgenovskie tranzienty, u kotoryh donorom yavlyaetsya zvezda-sverhgigant. A vo-vtoryh, sistemy s ochen' bol'shim poglosheniem, prichem pogloshenie svyazano imenno s samimi sistemami, a ne nabiraetsya po doroge. V stat'e daetsya podrobnyi obzor po etim sistemam, a takzhe kratko opisyvayutsya vazhnye dlya ponimaniya voprosy. arxiv:0809.1105 Katalog tochechnyh rentgenovskih istochnikov po dannym dvuhmegasekundnyh nablyudenii galakticheskogo centra na Chandre (A Catalog of X-ray Point Sources from Two Megaseconds of Chandra Observations of the Galactic Center) Authors: M. P. Muno et al. Comments: 23 pages, 13 figures, 7 tables. Submitted to ApJ Supplements Slozhiv dannye mnogih nablyudenii oblasti galakticheskogo centra, avtory poluchili zamechatel'nyi obzor ploshadki razmerom primerno 2 (po dolgote) na 0.8 gradusov. Tam vydeleno 9017 tochechnyh istochnikov. Provedena ih pervichnaya klassifikaciya. Interesno, po moim prikidkam, tam dolzhno byt' neskol'ko odinochnyh akkreciruyushih neitronnyh zvezd. Vot by ih vydelit'! arxiv:0809.1230 Registraciya zaderzhannogo gamma-izlucheniya ot GRB 080514B na AGILE (AGILE detection of delayed gamma-ray emission from GRB 080514B) Authors: A. Giuliani et al. Comments: 4 pages, A&A letters, in press Zabavno, posle uspeshnogo zapuska GLAST uchenye, rabotayushie s dannymi AGILE, tut zhe nachali vydavat' stat'i. Vot eshe odna. So vremen raboty pribora EGRET na bortu Komptonovskoi observatorii ne bylo registracii otnositel'no pozdnego (zaderzhannogo) izlucheniya gamma-vspleskov na ochen' bol'shih energiyah. AGILE optimizirovan dlya takih nablyudenii. I vot ot GRB 080514B zaregistrirovan potok na energiyah vyshe neskol'kih desyatkov MeV uzhe posle togo, kak ischez potok na standartnyh dlya gamma-vspleskov energii. Pravda, rech' idet o sekundah. Vsplesk dlilsya 7 sekund, a eshe 6 sekund posle etogo prihodili zhestkie kvanty. arxiv:0809.1280 Massivnaya dvoinaya iz dvuh chernyh dyr v OJ287 i testy obshei teorii otnositel'nosti (A massive binary black-hole system in OJ287 and a test of general relativity) Authors: M. J. Valtonen et al. Comments: 14 pages, 3 figures, published in Nature Lyubopytnyi rezul'tat. V kvazare OJ287 nablyudayutsya periodicheskie vspyshki s periodom 12 let (dve vspyshki za period). Schitaetsya, chto eto svyazano s sushestvovaniem tam dvoinoi chernoi dyry. Yasno, chto, vrashayas' drug vokrug druga, chernye dyry, soglasno OTO, dolzhny izluchat' gravvolny i sblizhat'sya. Poslednyuyu vspyshku (sentyabr' 2007) udalos' predskazat' s tochnost'yu do dnya. Esli by ne bylo gravvoln, to vspyshka proizoshla by na 20 dnei pozzhe. Model' dlya takogo povedeniya kvazara dvoe iz avtorov obsuzhdaemoi stat'i predlozhili eshe v 1996 godu. Odna iz chernyh dyr dva raza za period peresekaet akkrecionnyi disk vokrug vtoroi, chto i privodit k vspyshkam. Otmechu, chto vse-taki eto lish' odno iz vozmozhnyh ob'yasnenii. Sam istochnik byl izvesten kak peremennaya zvezda eshe v 19 veke, v 1968 g. on byl identificirovan kak kvazar, tak chto statistika po nablyudeniyam ego vspyshek nabralas' uzhe poryadochnaya. No lish' v proshlom godu dannyh okazalos' dostatochno, chtoby popytat'sya s tochnost'yu do neskol'kih dnei predskazat' sleduyushuyu vspyshku (skazhem, v 1996 godu avtory eshe ne mogli eto sdelat'). Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. obzor arxiv:0809.1602 Gravitacionno-volnovaya astronomiya (Gravitational Wave Astronomy) Authors: Kostas D. Kokkotas Comments: 22 pages, 2 figures Horoshii obzor, ohvatyvayushii vse osnovnye voprosy, svyazannye s gravitacionno-volnovoi astronomiei, krome teh, chto svyazany s konkretnymi ustanovkami. Rassmotreny osnovy fiziki gravvoln, istochniki, principy registracii. arxiv:0809.1648 Otkrytie neobychnogo opticheskogo tranzienta s pomosh'yu Kosmicheskogo teleskopa imeni Habbla (Discovery of an Unusual Optical Transient with the Hubble Space Telescope) Authors: K. Barbary et al. Comments: 5 pages, 4 figures. Accepted for publication in ApJ. V processe poiska i issledovaniya sverhnovyh v skopleniyah galaktik na Kosmicheskom teleskope obnaruzhilos' nechto, na sverhnovye ne slishkom pohozhee. Avtory raportuyut ob otkrytii opticheskogo tranzienta, kotoryi v techenie 100 dneya yarchal, dostignuv 21-i velichiny, a potom na primerno takom zhe masshtabe vremeni zatuh. Takaya krivaya bleska sovsem ne pohozha na sverhnovye ili drugie izvestnye tranzienty. Na meste "vspyshki" nichego ne vidno. Na mikrolinzirovanie tozhe ne pohozhe (etot vyvod sdelan po krivoi izmeneniya bleska). Sootvetstvenno, avtory polagayut, chto otkryli nechto, s chem ran'she my ne vstrechalis'. Pro rasstoyanie do ob'ekta pochti nichego ne izvestno. Krasnoe smeshenie opredelit' ne udalos' (net nikakih spektral'nyh detalei, kotorye by govorili o nenulevom smeshenii). No mozhno v lyubom sluchae postavit' zhestkii predel, chto ono men'she 2.7. Esli ob'ekt blizkii, to mozhno postavit' nizhnii predel na rasstoyanie, uchtya, chto ne byl obnaruzhen parallaks. Eto otodvigaet ob'ekt na 40 pk. T.e., eto uzh kak minimum ne Solnechnaya sistema. "Bol'she ne znayut o nem nichego" (s) Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. arxiv:0809.1678 Udarnaya volna ot vzryva Eta Kilya 1843 goda (A Blast Wave from the 1843 Eruption of Eta Carinae) Authors: Nathan Smith Comments: 10 pages, 3 color figs, supplementary information. Accepted by Nature V 1843 godu ot yarkoi zvezdy Ety Kilya nablyudalas' moshnaya vspyshka. V stat'e avtor rasskazyvaet o tom, chto im obnaruzheno bystro dvigayusheesya veshestvo (3500-6000 km v sek), svyazannoe s etoi vspyshkoi. Do etogo ranblyudalis' lish' sushestvenno men'shie skorosti. Novye dannye govoryat v pol'zu togo, chto vydelenie energii proizoshlo gluboko pod poverhnost'yu. A ran'she schitalos', chto nablyudaemyi razlet veshestva svyazan lish' s rezkim usileniem zvezdnogo vetra. miniobzor arxiv:0809.1800 Obrazovanie i evolyuciya kataklizmicheskih peremennyh (Formation and Evolution of Cataclysmic Variables) Authors: H. Ritter Comments: 14 pages, to appear in Mem. Soc. Astron. Italiana, Proceedings of the School of Astrophysics "Francesco Lucchin"; Nebol'shoi obzor po teme. My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing). arxiv:0809.0857 Lord Rezerford, ego nobelevskaya premiya 1908 goda po himii, i pochemu on ne poluchil vtoruyu premiyu (Lord Rutherford of Nelson, His 1908 Nobel Prize in Chemistry and Why He Didn't Get a Second Prize) Authors: C. Jarlskog Comments: 22 pages, Extended version of an invited talk presented at the neutrino conference "Neutrino 2008", Christchurch, New Zealand, 25-31 May 2008 Lyubopytnaya stat'ya o Rezerforde. V chastnosti, lyubopytno, chto na nobelevskie premii ego nominirovali v osnovnom uchenye iz Germanii, i ne nominirovali - iz Velikobritanii. Vernut'sya k nachalu stranicy

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