1998BaltA...7..269S


Query : 1998BaltA...7..269S

1998BaltA...7..269S - Baltic Astronomy, 7, 269-275 (1998/April-0)

Modeling of the accretion disc spectra in AM CVn systems.

SEMIONOVAS D.

Abstract (from CDS):

An attempt has been made to model the helium accretion disk with parameters expected for AM CVn type systems. In the spectrum of such a system we expect to see signatures of all its parts: the central white dwarf, the degenerate secondary, the disk and the wind. Spectral modeling of each component allows us to determine the properties of the system, which could help to understand the evolution of this particular type of cataclysmic variables. The theoretical spectra are compared to the observed spectra of AM CVn and V803 Cen.

Abstract Copyright: ∼

Journal keyword(s): stars: close binaries, cataclysmic variables, accretion disks - stars: individual (AM CVn, V803 Cen)

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PHL 1475 CV* 03 10 32.7677788896 -09 45 06.178429764           DB+ 100 0
2 V* AM CVn CV* 12 34 54.6231062664 +37 37 44.120620056   14.02 14.13 14.47   DBnnp 434 0
3 G 61-29 CV* 13 05 42.4009686696 +18 01 03.763561619   16.059 16.101 15.825   DBe 284 0
4 V* V803 Cen CV* 13 23 44.5389056832 -41 44 29.446810404   16.8 14.42     ~ 155 0
5 V* CR Boo CV* 13 48 55.2218717736 +07 57 35.724118680     15.00     ~ 185 0
6 V* HP Lib CV* 15 35 53.0715009672 -14 13 12.215196048   13.55       Bpec 112 0

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