Number of the records: 1  

Predicting the next outbursts of OJ 287 in 2006-2010

  1. 1.
    SYSNO ASEP0049429
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitlePredicting the next outbursts of OJ 287 in 2006-2010
    TitlePředpovídání dalších výbuchů OJ 287 v roce 2006- 2010
    Author(s) Valtonen, M.J. (FI)
    Lehto, H.J. (FI)
    Sillanpää, A. (FI)
    Nilsson, K. (FI)
    Mikkola, S. (FI)
    Hudec, René (ASU-R) RID, ORCID
    Bašta, Milan (ASU-R)
    Teräsranta, H. (FI)
    Haque, S. (TT)
    Rampadarath, H. (TT)
    Source TitleAstrophysical Journal - ISSN 0004-637X
    Roč. 646, č. 1 (2006), s. 36-48
    Number of pages13 s.
    Languageeng - English
    CountryUS - United States
    Keywordsquasars general ; quasars OJ 287
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsIAA3003206 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    AnnotationIn its nearly regular cycle of outbursts the quasar OJ 287 is due for another outburst season in 2006–2010. The prediction for the exact timing depends on the adopted model. In the precessing binary model of Lehto and Valtonen the timing depends on the time delay between the impact on the primary disk and the time when the impacted gas becomes optically thin. The time delay in turn depends on the properties of the accretion disk, the accretion rate, and the viscosity parameter α, which are not exactly known. We study the flexibility in timing provided by the uncertainties.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2007
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.