Physics – Plasma Physics
Scientific paper
Apr 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1121...22t&link_type=abstract
SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP Conference Proceedings, Volume 1121, pp. 22-27 (2009).
Physics
Plasma Physics
Giant And Subgiant Stars, Accretion And Accretion Disks, Mass Loss And Stellar Winds, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays, Astronomical And Space-Research Instrumentation, Ephemerides, Almanacs, And Calendars
Scientific paper
High resolution observations in the region of the lines Hα and Hγ of the spectrum of the symbiotic binary Z And were performed during its small amplitude brightening at the end of 2002. The profiles of the two lines were double-peaked and the velocity of the dip between the two peaks was the same. This behavior was interpreted with emission mainly of an optically thin accretion disc. The Hα line had broad wings which were supposed to be due to high velocity stellar wind. The line Hγ had a broad emission component which was thought to be emitted by an optically thin accretion disc or a high velocity stellar wind.
Bisikalo Dimitry V.
Tomov N. A.
Tomova M. T.
No associations
LandOfFree
Evidences for an Accretion Disc in the Spectrum of the Symbiotic Binary Z And during its Outburst at the end of 2002 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Evidences for an Accretion Disc in the Spectrum of the Symbiotic Binary Z And during its Outburst at the end of 2002, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidences for an Accretion Disc in the Spectrum of the Symbiotic Binary Z And during its Outburst at the end of 2002 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1861068