... Klochkova V.G., Chentsov E.L. The kinematics of an envelope of V510Pup - a core of a future planetarynebula. Astron. ... Astron. Letters, 2003, v. 29, p.842-857. Klochkova V.G., Panchuk V.E. From a star to a planetarynebula. Priroda. 2002. No.3. ...
... Klochkova V.G., Chentsov E.L. The kinematics of an envelope of V510Pup - a core of a future planetarynebula. Astron. ... A . v.388, p.563. Klochkova V., Panchuk V. From a star to a planetarynebula. Priroda. 2002, N3, p.28. ...
... We have discovered a planetarynebula in KKR25. ... This is the first known planetarynebula in a dwarf spheroidal galaxy outside the Local Group. ...
... of transition from AGB to a planetarynebula are commonly called postAGB objects or ... of IRAS 19475 suggests that the object is close to the planetarynebula stage ...
... photometric observations of the future planetarynebula IRAS18062+2410=V886Her in ... v.388, p.563 . Klochkova V., Panchuk V. From a star to a planetarynebula. Priroda. ...
... The atlas includes V1853 Cyg, IRAS18062+2410, MWC162 and the central star of the planetarynebula NGC6543. ... of the spectroscopic monitoring of a poorly-studied proto-planetarynebula (PPN) candidate IRAS01005+7910 at the 6-m telescope ...
... Introduction Intermediate-mass stars (with initial masses of 3 - 8 M ) that evolve from the asymptotic giant branch (AGB) to a planetarynebula (PN) are observed at the short proto-planetarynebula (PPN) phase. ...
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Ссылки http://mavr.sao.ru/hq/ssl/gvard/Nasonov-YSC17.proc.03-IR01005.pdf -- 428.3 Кб -- 01.11.2012 Похожие документы
... A the planetarynebula Mz3 ("Ant nebula"), B protoplanetary nebula RAFGL 2688, C WolfRayet star WR124, D LBV star Car, E Herbig Ae/Be stars, F T Tauri Using C M F G E N code we constructed the model of the WR156 atmosphere, the parameters are ...
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Ссылки http://mavr.sao.ru/hq/ssl/maryeva/WR156_poster_2014_eng.pdf -- 1081.4 Кб -- 16.06.2014 Похожие документы
... The development of such asphericities close to the central star suggests that CIT 3 is in the very end of its AGB evolution or even in transition to the proto-planetarynebula phase where most objects are observed in axisymmetric geometry. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2002/Hal_IAU209.ps -- 60.2 Кб -- 03.08.2004 Похожие документы