Search results

  1. 1.
    0354857 - ASÚ 2011 RIV FR eng J - Journal Article
    Kubát, Jiří - Saad, S.M. - Kawka, Adela - Nouh, M. I. - Iliev, L. - Uytterhoeven, K. - Korčáková, Daniela - Hadrava, Petr - Škoda, Petr - Votruba, Viktor - Dovčiak, Michal - Šlechta, Miroslav
    Spectroscopic analysis of the B/Be visual binary HR 1847.
    Astronomy & Astrophysics. Roč. 520, Sep-Oct (2010), A103/1-A103/17. ISSN 0004-6361. E-ISSN 1432-0746
    R&D Projects: GA ČR GA205/08/0003
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : Be stars * emission-line
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 4.410, year: 2010
    Permanent Link: http://hdl.handle.net/11104/0193766
     
     
  2. 2.
    0337551 - ASÚ 2010 RIV NL eng J - Journal Article
    Saad, S.M. - Kubát, Jiří - Nouh, M. I. - Hamdy, M.A.
    On correlation of H alpha, iron and oxygen line strengths in some B, Be and shell stars.
    Astrophysics and Space Science. Roč. 325, č. 1 (2010), s. 7-14. ISSN 0004-640X. E-ISSN 1572-946X
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : stars * Be and shell stars
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 1.437, year: 2010
    Permanent Link: http://hdl.handle.net/11104/0181519
     
     
  3. 3.
    0048011 - ASÚ 2007 RIV FR eng J - Journal Article
    Saad, S.M. - Kubát, Jiří - Korčáková, Daniela - Koubský, Pavel - Škoda, Petr - Šlechta, Miroslav - Kawka, Adela - Budovičová, Andrea - Votruba, V. - Kotková, Lenka - Nouh, M. I.
    Observations of Hα, iron, and oxygen lines in B, Be, and shell stars.
    [Pozorování čar Hα, železa a kyslíku v B, Be, a shell hvězdách.]
    Astronomy & Astrophysics. Roč. 450, č. 1 (2006), s. 427-430. ISSN 0004-6361. E-ISSN 1432-0746
    R&D Projects: GA ČR GA205/02/0445; GA ČR GA102/02/1000
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : line profiles * emission line Be * circumstellar matter
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 3.971, year: 2006
    Permanent Link: http://hdl.handle.net/11104/0138758
     
     


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