Academic Journal

Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Rapid variability of accretion in AM Herculis

التفاصيل البيبلوغرافية
العنوان: Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Rapid variability of accretion in AM Herculis
المؤلفون: D. De Martino, G. Matt, B. T. Gänsicke, R. Silvotti, J. M. Bonnet-bidaud, M. Mouchet
المساهمون: The Pennsylvania State University CiteSeerX Archives
المصدر: http://arxiv.org/pdf/astro-ph/0209538v1.pdf.
سنة النشر: 2002
المجموعة: CiteSeerX
الوصف: We present the last pointed observation of AMHer carried out during the life of the BeppoSAX satellite. It was bright at the beginning of the observation, but dropped to the lowest X-ray level ever observed so far. The X-ray emission during the bright period is consistent with accretion occurring onto the main pole of the magnetized white dwarf. The rapid change from the active state to the low deep state indicates a drop by a factor of 17 in the accretion rate and hence that accretion switched-off. The short timescale (less than one hour) of this variation still remains a puzzle. Optical photometry acquired simultaneousy during the low state shows that the white dwarf remains heated, although a weak emission from the accretion stream could be still present. Cyclotron radiation, usually dominating the V and R bands, is negligible thus corroborating the possibility that AMHer was in an off-accretion state. The X-ray emission during the inactive state is consistent with coronal emission from the secondary late type star.
نوع الوثيقة: text
وصف الملف: application/pdf
اللغة: English
Relation: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.314.8038; http://arxiv.org/pdf/astro-ph/0209538v1.pdf
الاتاحة: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.314.8038
http://arxiv.org/pdf/astro-ph/0209538v1.pdf
Rights: Metadata may be used without restrictions as long as the oai identifier remains attached to it.
رقم الانضمام: edsbas.FC6F55B9
قاعدة البيانات: BASE