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Physical processes in the very slow symbiotic nova PU Vul - possible triple system

  1. TitlePhysical processes in the very slow symbiotic nova PU Vul - possible triple system
    Author Chochol Drahomír 1947- SAVASTRO - Astronomický ústav SAV    ORCID
    Co-authors Pribulla Theodor 1970- SAVASTRO - Astronomický ústav SAV    ORCID

    Tamura Shinichi

    Tajitsu Akito

    Kanamitsu Osamu

    Source document / Mikolajewska Joanna Physical Processes in Symbiotic Binaries and Related Systems. P. 127-132. - Warsaw : CFPA, 1997 ; Physical processes in symbiotic binaries and related systems
    Languageeng - English
    CountryPL - Poland
    Document kindrozpis článkov z periodík (rzb)
    CitationsBELCZYNSKI, K - MIKOLAJEWSKA, J - MUNARI, U - IVISON, RJ - FRIEDJUNG, M. A catalogue of symbiotic stars. In ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES. ISSN 0365-0138, 2000, vol. 146, no. 3, pp. 407-435.
    HACHISU, I - KATO, M. The nature of premaximum halts of classical nova outbursts: V723 Cassiopeiae and V463 Scuti. In ASTROPHYSICAL JOURNAL. ISSN 0004-637X, 2004, vol. 612, no. 1, pp. L57-L60.
    IKEDA, Y - TAMURA, S. Spectroscopic diagnostics of symbiotic stars. II. Statistical analyses of highly resolved emission-line profiles. In PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. ISSN 0004-6264, 2004, vol. 56, no. 2, pp. 353-379.
    YOO, K.H. Nebular spectrum of PU Vul in 2004. In JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY. ISSN 0253-3065, 2007, vol. 40, no. 2, p. 39-47.
    CategoryAEC - Scientific papers in foreign peer-reviewed proceedings, monographs
    Category of document (from 2022)V2 - Vedecký výstup publikačnej činnosti ako časť editovanej knihy alebo zborníka
    Type of documentpríspevok
    Year1997
    article

    article

    rok vydaniarok metrikyIFIF Q (best)SJRSJR Q (best)
    1997
Number of the records: 1  

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