IW Andromedae
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 01h 01m 08.907s[2] |
Declination | 43° 23′ 25.79″[2] |
Apparent magnitude (V) | 13.7 to 17.3[3] |
Characteristics | |
Spectral type | sdOB[4] |
Variable type | Z Cam(?)[3]
|
Details | |
White dwarf | |
Mass | 0.75[5] M☉ |
Radius | 0.015[5] R☉ |
Temperature | 25,000[5] K |
Donor star | |
Mass | 0.27[5] M☉ |
Database references | |
SIMBAD | data |
IW Andromedae is a
The irregular variability of this star was discovered by
This is a close binary system with an
mass of the Sun. The secondary component has 27% of the Sun's mass and is overflowing its Roche lobe, resulting in mass transfer to an accretion disk orbiting the primary. The accretion rate for the primary is 3×10−9 M☉·yr−1.[5]
T. Kato and associates in 2003 found the light curve matched a Z Cam variable, with the previously observed inactive states being caused by a characteristic standstill. The duty cycle of its standstill is unusually long for a variable of this class.[10] Outbursts during these standstills may be explained by flares on the secondary, which result in brief surges in mass transfer.[12]
Other variables displaying IW And–type behavior have since been discovered, including HO Puppis,[13] BC Cassiopeiae,[14] IM Eridani, V507 Cygni, and FY Vulpecula.[7]
References
- ^ "Download Data", aavso.org, AAVSO, retrieved 9 April 2023.
- ^ .
- ^ S2CID 125853869.
- Bibcode:1980IBVS.1795....1M.
- ^ S2CID 118631716.
- ^ "IW ANd". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-04-07.
- ^ , 20.
- Bibcode:1975MitVS...7....1M.
- ^ S2CID 122899189.
- ^ Bibcode:2003IBVS.5376....1K.
- Bibcode:1987IBVS.3081....1M.
- S2CID 119238557, A48.
- S2CID 231979353, 51.
- , 98.