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  • 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"

  • astro-ph/0607173
    Dolgoperiodicheskii sil'no peremennyi rentgenovskii istochnik v molodom ostatke sverhnovoi
  • astro-ph/0607501
    Neuzheli my otkryli samyi yarkii UMI?
  • astro-ph/0607632
    Habblovskoe ul'traglubokoe pole
  • astro-ph/0607640
    Parksovskii mnogopuchkovyi obzor neba. VI. Otkrytie i taiming 142 pul'sarov i populyacionnyi sintez galakticheskih pul'sarov

    Otdel'nye stat'i
  • OT 060420: veroyatnyi opticheskii tranzient, zaregistrirovannyi obzornymi kamerami
  • Nablyudaya temnuyu storonu
  • Kosmicheskie luchi: nedavnii progress i tekushie problemy
  • Mnozhestvo dvoinyh sredi NEA
  • Dolgoperiodicheskii sil'no peremennyi rentgenovskii istochnik v molodom ostatke sverhnovoi
  • Svyazany li Proksima i Al'fa Centavra?
  • Izuchenie na Spitcere komet 2P/Encke, 67P/Churyumov-Gerasimenko i C/2001 HT50 (LINEAR-NEAT)
  • Izobrazheniya planetnogo kompan'ona molodogo burogo karlika 2MASS J1207334-393254 po dannym HST NICMOS
  • Katalog blizkih ekzoplanet
  • Neuzheli my otkryli samyi yarkii UMI?
  • Rentgenovskii spektr 10.6-sekundnogo pul'sara v Westerlund 1 po dannym Chandra
  • Rassmatrivaya nebo glazami Habbla: COSMOS SkyWalker
  • Poisk pul'sacii v radiodiapazone ot chetyreh anomal'nyh rentgenovskih pul'sarov i otkrytie dvuh novyh pul'sarov
  • Rentgenovskie dvoinye
  • Habblovskoe ul'traglubokoe pole
  • Raspredelenie mezhzvezdnoi sredy v Mlechnom Puti. Trehmernaya krupnomasshtabnaya model'
  • Parksovskii mnogopuchkovyi obzor neba. VI. Otkrytie i taiming 142 pul'sarov i populyacionnyi sintez galakticheskih pul'sarov


    Iz razdela physics
  • Proekt EEE
  • O dostupnyh lunnyh i solnechnyh zatmeniyah i vavilonskoi hronologii
  • Citirovanie kak process predstavleniya
  • Masshtabirovanie h-indeksa dlya razlichnyh razdelov ISI


    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.
  • Obzory preprintov astro-ph

    Vypusk N138
    astro-ph za 01 - 31 iyulya 2006 goda: izbrannye stat'i

    Referaty otdel'nyh statei



    astro-ph/0607033 OT 060420: veroyatnyi opticheskii tranzient, zaregistrirovannyi obzornymi kamerami (OT 060420: A Seemingly Optical Transient Recorded by All-Sky Cameras)
    Authors: Lior Shamir, Robert J. Nemiroff
    Comments: 21 pages, 7 figures, 3 tables, accepted PASP

    Kak izvestno, nauka ne zanimaetsya chudesami, t.e. nevosproizvodimymi yavleniyami. V astronomii v takuyu kategriyu mogut popadat' ochen' bystrye sobytiya, kotorye ne uspevayut kak sleduet rassmotret'. Odnako uchenye delayut vse, chto v ih silah, chtoby reshit' etu problemu.

    Sredi vozmozhnyh "chudes" mogut byt' ochen' bystrye tranzienty, dazhe v opticheskom diapazone. Poiskom takih sobytii zanimayutsya s pomosh'yu ochen' shirokougol'nyh kamer. 20 aprelya etogo goda dve kamery (odna v Chili, drugaya - v Ispanii) zaregistrirovali yarkuyu (5-ya velichina) vspyshku dlitel'nost'yu okolo 10 minut. Pervichnyi analiz pokazal, chto sobytie dolzhno byt' svyazano s astronomicheskim ob'ektom. Odnako pozzhe okazalos', chto sobytie ne bylo zaregistrirovano tret'ei kameroi. V dannoi stat'e avtory tshatel'no obsuzhdayut eto konkretnoe sobytie, a takzhe rassuzhdayut o tom, kak pravil'no iskat' podlinnye opticheskie tranzienty. Samo nablyudavsheesya sobytie avtory svyazyvayut s blikom ot kakogo-to kosmicheskogo musora.


    miniobzor astro-ph/0607066 Nablyudaya temnuyu storonu (Surveying the dark side)
    Authors: Roberto Trotta, Richard Bower
    Comments: 9 pages, no figures. Review article to appear in "Astronomy and Geophyiscs"

    Hotya Monti Paiton v lice Braiana i prizyvali nas smotret' na svetluyu storonu zhizni, tem ne menee nado pomnit' i o temnoi storone...

    Odnako ne stoit toropit'sya delat' mrachnoe lico, v dannom sluchae rech' idet vsego lish' ob issledovanii temnoi energii. Avtory dayut detal'nyi obzor tipov nablyudenii, kotorye mogut dat' kakuyu-to vazhnuyu informaciyu o svoistvah etogo komponenta vselennoi. Takzhe rassmatrivayutsya konkretnye proekty, kotorye v blizhaishee vremya dolzhny prolit' svet na temnuyu storonu.

    See you on the dark side of the Moon.

    And there is no dark side of the Moon really.


    miniobzor astro-ph/0607109 Kosmicheskie luchi: nedavnii progress i tekushie problemy (Cosmic Rays: Recent Progress and some Current Questions)
    Authors: A. M. Hillas
    Comments: 11 pages, 8 figures, Based on invited talk in "Cosmology, Galaxy Formation and Astroparticle Physics on the pathway to the SKA", Oxford, April 2006

    Ochen' emkii i udachnyi obzor po kosmicheskim lucham. Vsyacheski rekomenduetsya dlya oznakomleniya s sovremennym sostoyaniem del.


    astro-ph/0607128 Mnozhestvo dvoinyh sredi NEA (Many binaries among NEAs)
    Authors: David Polishook, Noah Brosch
    Comments: 5 pages, 2 figures, invited paper for NASA's "Near-Earth Object Detection, Characterization, and Threat Mitigation" workhop, Colorado, June 2006

    NEAs - Near Earth Asteroids. Stat'ya posvyashena ocenke doli dvoinyh ob'ektov sredi nih. Dolya okazyvaetsya velika. Esli v pervyh stat'yah rech' shla lish' o 15 procentah, potom o 50, to seichas avtory pishut o 2/3. Hotya zamechu, chto vyvody avtorov osnovyvayutsya na nebol'shom chisle izuchennyh ob'ektov, chto, na moi vzglyad, delaet prezhdevremennymi vyvody o tochnoi doli dvoinyh asteroidov, prohodyashih vblizi Zemli.


    astro-ph/0607173 Dolgoperiodicheskii sil'no peremennyi rentgenovskii istochnik v molodom ostatke sverhnovoi (A long-period, violently-variable X-ray source in a young SNR)
    Authors: A. De Luca, P.A. Caraveo, S. Mereghetti, A. Tiengo, G.F. Bignami
    Comments: Accepted for publication in Science. Published online via Science Express on 2006, July 6. 17 pages, 7 figures

    Kompaktnyi istochnik v ostatke sverhnovoi RCW 103 izvesten uzhe dostatochno davno. Tak zhe davno bylo yasno, chto on ne pohozh na "normal'nuyu" moloduyu neitronnuyu zvezdu. Vyskazyvalis' samye raznye gipotezy. Peremennost' istochnika, v svoyu ochered', tozhe ne yavlyaetsya novost'yu. I dazhe periodichnost' peremennosti uzhe obsuzhdalas', naprimer v rabotah G.G.Pavlova i ego kolleg. I vse-taki vot on - gvozd': detal'nye nablyudeniya na HMM-N'yutone pokazali nalichie chetkoi periodichnosti s periodom 6.67 chasa.

    Priroda istochnika po-prezhnemu ostaetsya neponyatnoi. To li eto dvoinaya sistema s malomassivnym kompan'onom (prisutstvie kompan'ona nikak v drugih diapazonah ne proyavlyaetsya), to li eto odinochnaya neitronnaya zvezda s anomal'no bol'shim (dlya takogo molodogo ob'ekta) periodom vrasheniya, to li chto-to eshe. Ne mogu ne vspomnit' svoyu staruyu ideyu o tom, chto istochnik yavlyaetsya "staroi" neitronnoi zvezdoi, a sam ostatok porozhden vzryvom kompan'ona po dvoinoi sisteme. Teper' zhe "staraya" neitronnaya zvezda akkreciruet vybroshennoe veshestvo. Pravda, period v chetvert' dnya tut takzhe ploho podhodit (pri takom periode orbital'naya skorost' slishkom velika, chtoby ozhidat' znachimoi akkrecii iz sredy vokrug). Mozhno postroit' model' v duhe "epiciklov", skazav, chto iznachal'no imelas' troinaya sistema (dve massivnye zvezdy i odna malomassivnaya). Massivnaya zvezda, vzrvavshayasya vtoroi, porodila nablyudaemyi ostatok, a pervaya porodila akkreciruyushuyu neitronnuyu zvezdu. Kak by to ni bylo, polagayu, chto ne stoit sbrasyvat' so schetov vozmozhnost', chto v kachestve rentgenovskogo istochnika my vidim ne tu zhe neitronnuyu zvezdu, chto porodila ostatok. Budem dumat' i zhdat'.


    astro-ph/0607401 Svyazany li gravitacionno Proksima i Al'fa Centavra? (Are Proxima and Alpha Centauri Gravitationally Bound?)
    Authors: Jeremy G. Wertheimer, Gregory Laughlin
    Comments: 10 pages total, 4 pages of text, 1 page of references, 3 figures, and 2 tables This article will be published in The Astronomical Journal

    Okazyvaetsya, chto vopros etot ne tol'ko do sih por ne reshen, no dlya ego razresheniya nuzhny novye bolee tochnye nablyudeniya! Delo v tom, chto Proksima slishkom daleka ot pary zvezd, sostavlyayushih Al'fu Centavra. Rasstoyanie kak raz poryadka togo, na kotorom prilivnoe deistvie Galaktiki mozhet razrushit' sistemu. Veroyatno, chto Proksima seichas nahoditsya v apoastre svoei orbity, no mozhet byt', chto vse-taki tri zvezdy ne obrazuyut edinuyu sistemu. Tak chto bez novyh nablyudenii ne oboitis'.


    astro-ph/0607416 Izuchenie na Spitcere komet 2P/Encke, 67P/Churyumov-Gerasimenko i C/2001 HT50 (LINEAR-NEAT) (A Spitzer Study of Comets 2P/Encke, 67P/Churyumov-Gerasimenko, and C/2001 HT50 (LINEAR-NEAT))
    Authors: Michael S. Kelley et al.
    Comments: Accepted for publication in the Astrophysical Journal 48 pages, 15 figures, 10 tables

    Hotya kosmicheskii infrakrasnyi teleskop imeni Spitcera byl sozdan v pervuyu ochered' dlya izucheniya zvezdoobrazovaniya i kosmologicheskih issledovanii, ego primenyayut i dlya nablyudenii ob'ektov Solnechnoi sistemy, naprimer komet.

    V stat'e privodyatsya dannye nablyudenii treh komet, dostatochno blizkih k Solncu (i Zemle) na moment nablyudeniya. Nikakih superkrasivyh kartinok net, zato est' dannye po chasticam v golovah komet i po ih yadram.


    astro-ph/0607490 Izobrazheniya planetnogo kompan'ona molodogo burogo karlika 2MASS J1207334-393254 po dannym HST NICMOS (HST NICMOS Imaging of the Planetary-mass Companion to the Young Brown Dwarf 2MASS J1207334-393254)
    Authors: Inseok Song et al.
    Comments: 18 pages, 3 figures, 3 tables. Accepted in ApJ

    Pod nomerom vosem' v proshlogodnii spisok samyh vazhnyh astronomicheskih otkrytii (po publikaciyam v Arhive) ya vnes obnaruzhenie planetnogo sputnika u burogo karlika. Sushestvennym momentom yavlyaetsya to, chto udalos' poluchit' pryamoe izobrazhenie planety (ob etom takzhe mozhno prochest' v iyul'skom nomere "Vokrug Sveta").

    Pervoe izobrazhenie bylo polucheno eshe v 2004 g., no tol'ko v 2005 byli polucheny podtverzhdeniya togo, chto dva ob'ekta (planeta i karlik) obrazuyut paru. Teper' zhe po novym dannym udalos' utochnit' rasstoyanie do sistemy (ono sostavlyaet 59+/-7 parsek) i rasstoyanie mezhdu komponentami (46+/-5 a.e. - eto v proekcii). Avtory eshe raz podcherkivayut, chto mozhno schitat' dokazannym, chto my imeem pervoe izobrazhenie vnesolnechnoi planety.


    astro-ph/0607493 Katalog blizkih ekzoplanet (Catalog of Nearby Exoplanets)
    Authors: R. P. Butler et al.
    Comments: 45-page preprint version. Published 2006 ApJ, 646, 505

    Sobstvenno, opisan katalog, razmeshennyi na ExoPlanets.Org. On soderzhit dannye po ekzoplanetam, vrashayushimsya vokrug zvezd, nahodyashihsya menee chem v 200 parsekah ot nas. V katalog vklyucheno 172 ob'ekta.


    astro-ph/0607501 Neuzheli my otkryli samyi yarkii UMI? (Have we detected the most luminous ULX so far?)
    Authors: G. Miniutti et al.
    Comments: MNRAS Letters in press

    Ya uzhe rasskazyval ob ul'tramoshnyh rentgenovskih istochnikah (UMI). V etoi rabote avtory opisyvayut rezul'taty nedavnih nablyudenii na sputnike XMM-Newton. Issleduya spiral'nuyu galaktiku (bez mozhnogo zvezdoobrazovaniya, imeyushuyu naimenovanie MCG-03-34-63, oni obnaruzhili vneyadernyi istochnik, potok ot kotorogo sootvetstvuet bolometricheskoi izotropnoi svetimosti 3 1041 erg v sekundu. T.o., istochnik yavlyaetsya pretendentom na zvanie samogo moshnogo iz izvestnyh UMI. Esli ocenka svetimosti verna, to my dolzhny imet' delo s akkreciei na chernuyu dyru s massoi bolee 2300 solnechnyh mass.


    astro-ph/0607528 >Rentgenovskii spektr 10.6-sekundnogo pul'sara v Westerlund 1 po dannym Chandra" proverka magnitarnoi gipotezy (The Chandra X-ray Spectrum of the 10.6 s Pulsar in Westerlund 1: Testing the Magnetar Hypothesis)
    Authors: S.L. Skinner, R. Perna, S.A. Zhekov
    Comments: 20 pages, 5 figures; to appear in ApJ

    Proveden analiz dannyh rentgenovskih nablyudenii odnogo iz anomal'nyh rentgenovskih pul'sarov, nahodyashegosya v skoplenii Westerlund 1. Hotya po "pervichnym priznakam" ob'ekt pohozh na standartnye anomal'nye pul'sary, tem ne menee polnoi yasnosti net. Svetyat ochen' malen'kie "pyatna", i polnaya svetimost' pri etom na poryadok men'she, chem u drugih istochnikov dannogo tipa.


    astro-ph/0607529 Rassmatrivaya nebo glazami Habbla: COSMOS SkyWalker (Seeing the sky through Hubble's eye: The COSMOS SkyWalker)
    Authors: K. Jahnke, S. F. Sanchez, A. Koekemoer
    Comments: 4 pages, 2 figures, accepted for publication in PASP

    Rech', konechno, idet ne o glazah Edvina Habbla, a o Kosmicheskom teleskope ego imeni. Problema sostoit v tom, chto vizualizovat' na komp'yutere udalennuyu bazu dannym, soderzhashuyu habblovskie dannye, sovsem neprosto. Avtory opisyvayut metodiku, kotoraya pozvolila by dazhe bez ochen' bystroi svyazi prosmatrivat' na ekrane chasti bol'shogo izobrazheniya, razmerom poryadka milliarda pikselov.

    Stranica proekta nahoditsya zdes'.


    astro-ph/0607614 Poisk pul'sacii v radiodiapazone ot chetyreh anomal'nyh rentgenovskih pul'sarov i otkrytie dvuh novyh pul'sarov (Search for radio pulsations in four Anomalous X-ray Pulsars and discovery of two new pulsars)
    Authors: M. Burgay et al.
    Comments: 8 pages, 6 figures, accepted by MNRAS

    Avtory proveli poisk pul'siruyushego radioizlucheniya ot chetyreh anomal'nyh rentgenovskih pul'sarov: 1RXS J170849.0-400910, 1E1048.1-5937, 1E 1841-045, AX J1845-0258. Ni ot odnogo ne bylo obnaruzheno radioimpul'sov. Zato poputno udalos' otkryt' dva novyh radiopul'sara!

    Poisk provodilsya na vysokoi chastote (okolo 1300 MGc). Mozhet byt' v etom kroetsya prichina neudachi. Ved' poka zhe polozhitel'nogo rezul'taty udalos' dostich' tol'ko gruppe issledovatelei v Pushino, kotorye ot anomal'nogo rentgenovskogo pul'sara 1E 2259+586 smogli zaregistrirovat' pul'siruyushee radioizluchenie na nizkoi chastote (okolo 110 MGc). [Da eshe ot ARP XTE 1810-197 udalos' uvidet' radioizluchenie vo vremya aktivnoi fazy istochnika astro-ph/0605429]


    obzor astro-ph/0607624 Rentgenovskie dvoinye (X-ray binaries)
    Authors: H. Schatz, K. E. Rehm
    Comments: 23 pages, 1 figure, to appear in Nucl. Phys. A

    Obzor po rentgenovskim dvoinym s tochki zreniya yadernoi fiziki. Delo v tom, chto krome vydeleniya energii za schet akkrecii, v dvoinyh s kompaktnymi ob'ektami (v pervuyu ochered' s neitronnymi zvezdami) idet mnogo interesnyh yadernyh processov.

    Obzor ochen' ponyatnyi i dostupnyi: formul net, zato est' obshirnaya bibliografiya i opisanie fakticheskogo nablyudatel'nogo materiala. Rekomenduyu.


    astro-ph/0607632 Habblovskoe ul'traglubokoe pole (The Hubble Ultra Deep Field)
    Authors: Steven V. W. Beckwith, et al.
    Comments: 44 pages, 18 figures, to appear in the Astronomical Journal October 2006

    Predstavleny rezul'taty glubokogo snimka, poluchennogo na Kosmicheskom teleskope. Ekspoziciya sostavila odin million sekund! Nablyudalas' ploshadka ploshad'yu vsego lish' 11 kvadratnyh uglovyh minut. Predel'naya zvezdnaya velichina primerno ravna 29. Sostavlen katalog primerno 10 000 ob'ektov.


    astro-ph/0607638 Raspredelenie mezhzvezdnoi sredy v Mlechnom Puti. Trehmernaya krupnomasshtabnaya model' (The distribution of the ISM in the Milky Way A three-dimensional large-scale model)
    Authors: A. Misiriotis et al.
    Comments: 14 Pages, 10 figures

    Po dannym nablyudenii v mikronnom diapazone na COBE/DIRBE avtory stroyat trehmernuyu kartinu raspredeleniya gaza i zvezd v Galaktike. Krome togo, polucheny ocenki raspredeleniya tempa zvezdoobrazovaniya po radiusu.


    astro-ph/0607640 Parksovskii mnogopuchkovyi obzor neba. VI. Otkrytie i taiming 142 pul'sarov i populyacionnyi sintez galakticheskih pul'sarov (The Parkes multibeam pulsar survey: VI. Discovery and timing of 142 pulsars and a Galactic population analysis)
    Authors: D. R. Lorimer et al.
    Comments: 30 pages, 8 figures, 9 tables, accepted for publication in MNRAS

    Vo-pervyh, avtory opisyvayut svezheotkrytye pul'sary. Ih azh 142. T.o., polnoe chislo pul'sarov, otkrytyh v ramkah obzora, dostiglo 742!!! Vo-vtoryh, ispol'zuya polnye dannye po pul'saram, zadetektirovannym v ramkah proekta, avtory vychislyayut vazhnye parametry populyacii vcelom. V chastnosti temp rozhdeniya pul'sarov sostavlyaet 1.4+/-0.2 za sto let.




    My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing).


    physics/0607027 Proekt EEE (The EEE Project)
    Authors: R. Antolini et al.
    Comments: 4 pages, 29th International Cosmic Ray Conference Pune (2005) 8, 279-282

    EEE- ``Extreme Energy Events''. T.o., proekt posvyashen detektirovaniyu kosmicheskih luchei sverhvysokih energii. Ideya sostoit v ustanovke myuonnyh detektorov v ital'yanskih shkolah poslednei stupeni.


    physics/0607137 O dostupnyh lunnyh i solnechnyh zatmeniyah i vavilonskoi hronologii (On the Available Lunar and Solar Eclipses and Babylonian Chronology)
    Authors: V.G.Gurzadyan, D.A.Warburton
    Comments: Akkadica, v.126 (2005) p.195

    Kak horosho izvestno, mnogie vremennye shkaly v istorii "graduiruyutsya" po astronomicheskim "veham". V dannom sluchae rech' idet o vavilonskoi istorii i nablyudeniyah Venery i zatmenii.

    Druguyu svezhuyu stat'yu po astronomicheskim metodam v hronologii drevnih epoh mozhno naiti zdes'.


    cs.DL/0607070 Citirovanie kak process predstavleniya (Citation as a Representation Process)
    Authors: V. V. Kryssanov, F. J. Rinaldo, H. Ogawa, E. Kuleshov
    Comments: 5 pages, 2 figures.

    Slegka zaumnyi podhod k voprosu o citirovanii. Avtory predlagayut novyi podhod k ponimaniyu samogo processa citirovaniya.


    physics/0607224 Masshtabirovanie h-indeksa dlya razlichnyh razdelov ISI (Scaling the h-index for different scientific ISI fields)
    Authors: Juan E. Iglesias, Carlos Pecharroman
    Comments: 7 pages

    Avtory obsuzhdayut, kak mozhno primenyat' h-indeks dlya uchenyh razlichnyh special'nostei.



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