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Soderzhanie i bystryi perehod k razdelam obzora
Novaya populyaciya korotkih gamma-vspleskov na bol'shih krasnyh smesheniyah Nablyudeniya effekta Askaryana vo l'du
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
Diskussii po stat'yam Arhiva
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Obzory preprintov astro-ph
Vypusk N144
astro-ph za 01 - 10 noyabrya 2006 goda: izbrannye stat'i
Referaty otdel'nyh statei
Authors: Ray Norris et al. Comments: 10 pages, Proceedings of Special Session SPS6 (Astronomical Data Management) at the IAU GA 2006. To appear in Highlights of Astronomy, Volume 14, ed. K.A. van der Hucht Sobstvenno, stat'ya predstavlyaet soboi daidzhest togo, chto rasskazyvalos' na special'noi sessii General'noi Assamblei MAS, posvyashennoi rabote s astronomicheskimi dannymi. My zhivem vo vremya, kogda potok dannyh chrezvychaino vozros. S drugoi storony, vozrosli i vozmozhnosti raboty s dannymi. Sootvetstvenno, vazhno prilozhit' um i ruki dlya togo, chtoby ispol'zovat' vsyu etu informaciyu s maksimal'noi pol'zoi. V stat'e, razumeetsya, rech' idet po nemnogu obo vsem. Zdes' i Virtual'naya observatoriya, i arhivy nablyudatel'nyh dannyh, i zhurnaly ... V obshem - polezno i dostatochno interesno.
Authors: R. E. Taam, P. M. Ricker Comments: 14 pages, 10 figures, to appear in proceedings of "A life with stars," a conference in honor of Ed van den Heuvel's 60th birthday, New Ast. Rev Bol'shoi obzor, posvyashennyi takoi vazhnoi stadii evolyucii tesnyh dvoinyh zvezdnyh sistem, kak "obshaya obolochka". Na etoi stadii proishodit sblizhenie komponent sistumy za schet unosa uglovogo momenta obolochkoi. Poterya veshestva svyazana s tem, chto odna iz zvezd uzhe sil'no proevolyucionirovala i ushla s glavnoi posledovatel'nosti. Itogom stadii mozhet stat' ili ochen' tesnaya dvoinaya, ili zhe komponenty prosto sol'yutsya. Nekotorye nablyudaemye tipy dvoinyh, a takzhe odinochnye zvezdy (naprimer, bystro vrashayushiesya giganty FK Coma) mogut obrazovyvat'sya, po vsei vidimosti, tol'ko v rezul'tate stadii s obshei obolochkoi.
Authors: E. Berger et al. Comments: 16 pages, Submitted to ApJ; 6 figures, 1 table; comments are welcome Predstavleny dannye opticheskih nablyudenii semi korotkih gamma-vspleskov. Dlya nekotoryh iz nih udalos' uvidet' opticheskie poslesvecheniya i obnaruzhit' materinskie galaktiki. Po vsei vidimosti, galaktiki eti nahodyatsya na krasnom smeshenii poryadka 1 ili dazhe bol'she. Eti dannye pozvolyayut avtoram sdelat' ryad vazhnyh ocenok i zaklyuchenii. Samoe sushestvennoe sostoit v tom, chto polnoe energovydelenie v etih vspleskah (v predpolozhenii izotropii) sushestvenno prevoshodit energiyu, vydelyaemuyu pri korotkih vspleskah na malyh krasnyh smesheniyah. Eto pozvolyaet govorit' o vozmozhnom vydelenii novoi populyacii korotkih gamma-vspleskov.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: Matthew G. Baring Comments: 13 pages, no figures. Invited review, accepted for publication in Astrophysics and Space Science, as part of the HEDLA 2006 conference proceedings Nesmotrya na tematiku obzor prakticheski ne soderzhit formul. Vse klyuchevye momenty razbirayutsya dostatochno populyarno. Obzor soderzhit bol'shoi spisok literatury s uporom na samye svezhie raboty, poetomu ego mozhno rekomendovat' kak horoshee vvedenie v temu.
Authors: Roberto Soria Comments: 4 pages, to appear in the proceedings of "Black Holes: from Stars to Galaxies", IAU Symp. No. 238, V. Karas & G. Matt eds., Cambridge University Press UMI - Ul'tramoshnye rentgenovskie istochniki. Situaciya s nimi tak poka i ne proyasnilas': to li eto akkreciruyushie chernye dyry promezhutochnyh mass, to li eti sistemy s "obychnymi" zvezdnymi chernymi dyrami. Absolyutno neponyatno, kak oni obrazuyutsya. Kak raz poslednei teme i posvyashen korotkii obzor. Stat'ya prekrasno strukturirovana. Dlya koroten'kogo obzora eto prakticheski obrazec.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: Charles D. Dermer Comments: 6 pages, 2 figures, in Proc. of TeV-Particle Astrophysics II, Madison, WI, 28-31 Aug, 2006 Poskol'ku est' nadezhda, chto v blizhaishie gody chuvstvitel'nost' detektorov budet dostatochnoi dlya registracii astrofizicheskih neitrino vysokih energii, aktual'no obsudit' naibolee perspektivnye istochniki. V ih chislo voshli gamma-vspleski, blizary, mikrokvazary i ostatki sverhnovyh.
Authors: The ANITA collaboration: S. W. Barwick et al. Comments: 4 pages, 5 figures Eshe v 1962 godu Askaryan opublikoval v ZhETF stat'yu, v kotoroi byl opisan effekt, kotoryi, pohozhe, privedet k poyavleniyu naibolee effektivnogo metoda registracii neitrino ochen'-ochen' vysokih energii (poryadka milliona TeV). Effekt byl eksperimental'no proveren v neskol'kih sredah, no bylo ochen' vazhno provesti proverku dlya l'da, ibo imenno v etoi srede stoyat prototipy budushih krupnyh detektorov. I vot, v rezul'tate oblucheniya semitonnoi glyby l'da, effekt proveren i dlya l'da.
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: B. N. Dwivedi Comments: 24 pages, 15 figures Solnechniki ne chasto baluyut chitatelei Arhiva, a tut srazu bol'shoi obzor. Stat'ya posvyashena poslednim dannym so sputnikov (Yohkoh, SOHO, TRACE, i RHESSI) s uporom na rezul'taty SOHO. Krasivye kartinki!
Obsudit' v ZhZh-soobshestve
ru_astroph.
Authors: S. Frey Comments: 8 pages; invited review, to appear in the Proceedings of the 8th European VLBI Network Symposium held in Torun, Poland, 26-29 September 2006. VLBI - eto interferometriya so sverhdlinnoi bazoi. Nablyudeniya provodyatsya, razumeetsya, v radiodiapazone. Itogom yavlyaetsya ochen' horoshee uglovoe razreshenie. V stat'e summiruyutsya obzornye nablyudeniya s pomosh'yu dannoi tehniki.
Authors: Myriam Gitti et al. Comments: 6 pages, 5 figures. To appear in the Proceedings of "Heating vs. Cooling in Galaxies and Clusters of Galaxies", August 2006, Garching (Germany) Zhelayushie pochitat' original'nyi material po etoi novosti priglashayutsya. Sut' tam takova, chto moshnoe aktivnoe yadro galaktiki vybrasyvaet strui dostatochnoi moshnosti, chtoby sushestvenno vliyat' na svoe okruzhenie v skoplenii galaktik.
Authors: Rob Fender et al. Comments: Accepted for publication in the proceedings of VI Microquasar Workshop: Microquasars and Beyond, 18-22 September 2006, Como (Italy), ed: T. Belloni (2006) LOFAR - eto grandioznyi proekt sistemy radioteleskopov. Pered takim moshnym instrumentom vsegda stavyat mnozhestvo zadach. Odna iz nih - radiomonitoring. V radiodiapazone ochen' trudno iskat' vspyhivayushie istochniki. Obychno v katalogi popadayut ob'ekty, izluchayushie postoyanno. Tol'ko v poslednie gody stali poyavlyat'sya tehnologii, pozvolyayushie reshit' etu problemu. Uzhe obnaruzheno neskol'ko zagadochnyh tipov radiotranzientov, o kotoryh my pisali v obzorah. Proekt po radiomonitoringu vhodit v chislo chetyreh prioritetnyh dlya LOFAR. Sootvetstvenno, mozhno ne somnevat'sya, chto posle vvoda ustanovok v stroi otkrytiya ne zamedlyat poyavit'sya.
My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing).
Authors: E. Peik, B. Lipphardt, H. Schnatz, Chr. Tamm, S. Weyers, R. Wynands Comments: 10 pages, 3 figures, Proceedings of the 11th Marcel Grossmann Meeting, Berlin, 2006 Astrofizicheskie testy postoyanstva fundamental'nyh konstant imeyut ochvidnoe preimushestvo: tam my operiruem v remenami poryadka milliardov let. Zato, laboratornye eksperimenty gorazdo tochnee i menee model'no-zavisimy! Issledovaniya atomnyh standartov na masshtabe neskol'kih let pozvolyaet sdelat' vazhnye ogranicheniya na variacii konstant. Tochnost' sravnima s astrofizicheskimi dannymi. Poka nichego ne obnaruzheno. Vse stabil'no.
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