Published 1985 | Version v1
Journal article

Statistical analysis of outbursts and superoutbursts of VW Hyi

Creators

  • 1. Polska Akademia Nauk, Warsaw (Poland). Centrum Astronomiczne

Description

The amplitude and width of normal outbursts of VW Hyi are correlated with the length of preceding cycle, but not with the length of following cycle. Two types of supercycles are identified: Type L, in which the average length of the last two cycles is longer than 30 days and Type S, in which it is shorter than 23 days. In Type L supercycles the mean length of cycle, the mean amplitude and width of outburst increase within supercycle with the consecutive number of cycle. In Type S supercycles, however, the last two cycles are short and the last outburst - much weaker. No obvious relation of the two types to other parameters of supercycles or superoutbursts seems to exist. The cycle-averaged outburst fluxes indicate a slight enhancement in the mass transfer rate immediately after superoutburst and confirm its major enhancements during outbursts which occur within 50 days of the next superoutburst. 12 refs., 5 figs., 1 tab. (author)

Additional details

Publishing Information

Journal Title
Acta Astronomica
Journal Volume
35
Journal Issue
3-4
Series
Acta Astron.
Journal Page Range
357-367
ISSN
0001-5237
CODEN
AASWA

INIS

Country of Publication
Poland
Country of Input or Organization
Poland
INIS RN
20082111
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ACCRETION DISKS; DWARF STARS; MASS TRANSFER; NOVAE; PHOTOMETRY; STAR ACCRETION; STAR BURNING; STAR MODELS
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; MATHEMATICAL MODELS; STAR EVOLUTION; STARS; VARIABLE STARS