Modelirovanie budushego chitat online dating

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Modelirovanie budushego chitat online dating

arxiv:0812.2561 Kratnos' zvezd s ekzoplanetami - novye malomassivnye zvezdnye komponenty u HD125612 i HD212301 (The multiplicity of exoplanet host stars - new low-mass stellar companions of the exoplanet host stars HD125612 and HD212301) Authors: M. Neuhauser Comments: 7 pages, A&A in press Obnaruzheny dva malomassivnyh (0.18 i 0.35 mass Solnca) sputnika u dvuh zvezd s ekzoplanetami. Eto uzhe 42-ya i 43-ya dvoinaya sistema s ekzoplanetami. Najarro Comments: 116 pages, A&A Reviews Ogromnyi obzor po potere veshestva massivnymi zvezdami. Budet kakoe-to vremya nastol'nym dlya vseh, kto s etim svyazan. Takie issledovaniya pozvolyayut luchshe ponyat', kak eti svetila ustroeny vnutri, a znachit, proverit' nashi teorii vnutrennego stroeniya zvezd.Odin iz nih (bolee massivnyi) nahoditsya vsego lish' v 230 a.e. No polezno znat', chto dazhe bez ucheta effektov selekcii okolo 17% ekzoplanetnyh sistem nahodyatsya v dvoinyh i kratnyh sistemah. arxiv:0811.1080 Seismologicheskaya programma Co Ro T (The seismology programme of Co Ro T) Authors: E. Poputno, konechno, mozhno poluchat' vsyakie drugie rezul'taty, naprimer, svyazannye s ekzoplanetami....a scientific method based on the importance of knowing yourself, and on what we are and what we're looking for. For this reason the suggested partners are always the outcome of a careful analysis on matching.The "starting from here" makes the relationship possible. Would you like to express yourself better, but don't know how? In a few steps you'll get your self-esteem and feel ready to break the ice!Krome opisaniya sobstvenno kompleksa zvezdoobrazovaniya v Orione avtor dostatochno detal'no opisyvaet odin iz scenariev formirovaniya poyasa Gulda, i voobshe kartinu nedavnego zvezdoobrazovaniya v solnechnoi okrestnosti. arxiv:0812.0482 Spektry belyh karlikov i modeli atmosfer (White dwarf spectra and atmosphere models) Authors: Detlev Koester Comments: 11 pages, to appear in Mem. Dumayu, chto seichas est' eshe bolee kachestvennye modeli (naprimer, u Suleimanova), no etot tekst polezen imenno kak sposob razobrat'sya v tom, chto i kak schitayut, a dal'neishie detali mozhno naiti po ssylkam. takzhe rabotu arxiv:0812.0491, v kotoroi obsuzhdayutsya effekty, vliyayushie na opredelenie mass belyh karlikov pri nizkoi temperature.arxiv:0812.1227 Nablyudaemye proyavleniya elementov r-processa v naibolee staryh zvezdah Galaktiki (Observing the Signatures of the r-Process in the Oldest Galactic Stars).V hode korotkih nablyudenii budet izucheno chut' bol'shee kolichestvo ob'ektov.Seichas missiya nahoditsya primerno v seredine svoego zhiznennogo cikla. arxiv:0811.15774 Issledovanie nizhnego predela na massu predsverhnovyh i massivnoi chasti sootnosheniya nachal'noi i konechnoi mass po dannym o belyh karlikah v rasseyannom skoplenii M35 (NGC2168) (Probing the lower mass limit for supernova progenitors and the high-mass end of the initial-final mass relation from white dwarfs in the open cluster M35 (NGC2168)) Authors: Kurtis A. Comments: 16 pages, accepted for publication in the Ap J Chasto mozhno prochest', chto "zvezdy, bolee legkie chem primerno 8-10 mass Solnca, v konce svoei evolyucii prevrashayutsya v belye karliki".

Authors: Carla Cacciari Comments: 10 pages, 2 figures, IAU Symp.258 on "The Ages of Stars" Evropeiskii kosmicheskii proekt Gaia, zaplanirovannyi k zapusku v 2011 godu, pozvolit poluchit' astrometricheskie, fotometricheskie i spektroskopicheskie dannye dlya bolee chem milliarda zvezd yarche 20-i zvezdnoi velichiny. 39-50 Sputnik Co Ro T uzhe pochti dva goda nahoditsya na orbite (s 26 dekabrya 2006 g.).V stat'e dano opisanie instrumenta, privodyatsya ego osnovnye harakteristiki i obsuzhdayutsya nauchnye napravleniya, v kotoryh Gaia pozvolit dostich' revolyucionnyh izmenenii. Osnovnaya zadacha sputnika - izuchenie pul'sacii zvezd - astroseismologiya.arxiv:0811.0487 Poterya massy massivnymi goryachimi zvezdami (Mass loss from hot massive stars) Authors: J. V stat'e daetsya obzor imenno astroseismologicheskih zadach i rezul'tatov missii.Osnovnye rezul'taty poluchayutsya v rezul'tate dolgih (chut' menee polugoda) nablyudenii odnoi ploshadki (razumeetsya, na nei mozhno izuchat' srazu neskol'ko ob'ektov). Krome etogo, provodyatsya korotkie (tri-chetyre nedeli) nablyudeniya.

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