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The R.A.P. Project (Reviews of Astro-Ph)

Mehanizmy izlucheniya, perenos izlucheniya


obzor! astro-ph/0207223 The Iron Project and Non-LTE stellar modeling
Author: Sultana N. Nahar
Comments: 15 pgs., 5 color figs., Invited Review, Proceedings of the Workshop on Stellar Atmosphere Modeling, Tuebingen, Germany, April 8-12, 2002

12 iyulya v astro-ph poyavilos' srazu tri raboty etogo avtora, posvyashennye atomnoi fizike. V dannom obzore avtor opisyvaet poslednie dostizheniya v vychislenii neprozrachnostei, chto yavlyaetsya chrezvychaino aktual'nym dlya astrofiziki (zvezdnye atmosfery, tumannosti, aktivnye yadra galaktik i t.d.).

Krome osnovnyh fizicheskih processov, sushestvennyh dlya dannyh vychislenii, i prochei "kuhni" avtor opisyvaet onlainovye bazy dannyh i dostupnye kody dlya sootvetstvuyushih vychislenii.

lekciya astro-ph/0208397 X- and Gamma-Ray Line Emission Processes
Authors: Vincent Tatischeff
Comments: 46 pages including 16 figures, uses eas.cls, to appear in the proceedings of the Aussois 2001 summer school "Stades Ultimes de l'Evolution Stellaire", EAS Pub. Series

V lekciyah opisyvayutsya razlichnye mehanizmy izlucheniya v liniyah v zhestkom diapazone (izluchenie goryachei plazmy, radioaktiyni raspad, annigilyaciya). Svoistva izlucheniya zatem obsuzhdayutsya v svete registracii na sovremennyh sputnikah. Navernoe seichas eto osobenno aktual'no v svyazi s gryadushim zapuskom sputnika Integral, 25 procentov nablyudatel'nogo vremeni kotorogo prinadlezhit Rossii.


astro-ph/0208542 A New Kinetic Equation for Compton Scattering
Authors: George B. Rybicki
Comments: 26 pages, 5 figures, submitted to ApJ

Daetsya novoe kineticheskoe uravnenie dlya komptonovskogo rasseyaniya (otlichnoe ot uravneniya Kompaneica). Pokazano, chto pri ispol'zovanii novogo uravneniya ne voznikaet bol'shih tehnicheskih trudnostei i pri etom daet bolee akkuratnye rezul'taty.


astro-ph/0209109 General Relativistic Magnetoionic Theory
Authors: Avery Broderick, Roger Blandford
Comments: To appear in the proceedings of the Amsterdam Circular Polarisation workshop

Razvit podhod dlya opisaniya perenosa izlucheniya v magnitoaktivnoi plazme s uchetom effektov OTO. Eto vazhno v pervuyu ochered' dlya rascheta akkrecionnyh potokov v okrestnostyah kompaktnyh ob'ektov (neitronnyh zvezd i chernyh dyr).


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obzor astro-ph/0210280 X-Ray Spectroscopy and Atomic Data
Authors: Ehud Behar, Steven M. Kahn
Comments: Review for proccedings of NASA Laboratory Astrophysics Workshop, May 1-3 2002, Farid Salama, Editor

Dlya razvitiya rentgenovskoi spektroskopii v astronomii (chto vazhno v svyazi s zapuskami takih sputnikov kak N'yuton i Chandra) neobhodimy i laboratornye issledovaniya. V stat'e opisyvayutsya eksperimenty Lourensovskoi Nacional'noi Laboratorii v Livermore. Osnovnye rezul'taty svyazany s issledovaniyami ionizirovannogo zheleza.


astro-ph/0212382 Radiativnyi cikl stimulirovannogo izlucheniya atomov (ionov) v astrofizicheskoi plazme (A Radiative Cycle with Stimulated Emission from Atoms (Ions) in an astrophysical Plasma)
Authors: S. Johansson, V. S. Letokhov
Commets: Accepted for publication in Phys. Rev. Letters

Rech' idet o lazernom izluchenii ot zvezdy Eta Kilya. Ob etom vy mozhete prochest' v stat'e " Eta Carinae - lazer, sozdannyi samoi prirodoi". Cikl sostoit ih 4 zven'ev - 4 urovnei i 4 perehodov mezhdu nimi v ionah odnokratno ionizirovannogo zheleza FeII (na risunke pokazany 2 blizkih cikla). Vozbuzhdenie cikla (perehod 1->4) proizvoditsya osnovnym izlucheniem zvezdy v linii L\alpha. Dlina volny L\alpha i perehoda 1->4 zametno ne sovpadayut. Odnako v opticheski plotnoi obolochke zvezdy L\alpha-fotony mnogokratno pereizluchayutsya i diffundiruyut po chastote iz-za effekta Dopplera. Perehody 4->3 i 2->1 - "obychnye" i proishodyat dostatochno bystro. A vot uroven' 3 (perehod 3->2) - metastabil'nyi. V sostoyanii 3 atomy sushestvuyut dostatochno dolgo v rezul'tate chego voznikaet inversnaya zaselennosti urovnei 2 i 3. Eto i est' "zvezdnyi lazer" - v obychnyh usloviyah liniya 3->2 ochen' slaba, no v radiativnom cikle chislo fotonov v etoi linii takoe zhe, kak i v ostal'nyh perehodah cikla.

astro-ph/0212529 Obnaruzhenie gigantskih impul'saov ot pul'sara PSR B1112+50 (Detection of Giant Pulses from the Pulsar PSR B1112+50)
Authors: A.A.Ershov, A.D.Kuzmin
Commets: 5 pages, 4 figures, to appear in: Pis'ma v Astronomicheskii Zhurnal, 2003, v.29, No.2, p111-115 and will be translated as: Astronomy Letters, v.29, No.2, p.91-95

Obnaruzheno, chto u pul'sara PSR B1112+50 primerno odin iz 150 impul'sov yavlyaetsya gigantskim: v 30 raz bolee intensivnym chem v srednem. Nablyudeniya provodilis' na Pushinskom radioteleskope BSA. Obsuzhdayutsya svoistva etih impul'sov.


astro-ph/0302190 Kovariantnaya magnitoionnaya teoriya I: rasprostranenie izlucheniya (Covariant Magnetoionic Theory I: Ray Propagation)
Authors: Avery Broderick, Roger Blandford (Caltech)
Commets: 12 pages, Submitted to MNRAS

Pervaya v serii statei, posvyashennyh opisaniyu rasprostraneniya izlucheniya v plazme astrofizicheskih ob'ektov s uchetom effektov OTO, STO, magnitnogo polya i t.d. Stat'ya ochen' tehnicheskaya, odnako, ochen' vazhnaya. V pervuyu ochered' ee rezul'taty prilozhimy k akkrecii na kompaktnye ob'ekty, chto avtory i pokazyvayut na nekotoryh primerah.


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