Light curves for M31-RV, adapted from Boschi and Munari (2004).[1] The red dots show the red band magnitude, and the blue dots show the blue band magnitude. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Andromeda |
Right ascension | 00h 43m 02.433s[2] |
Declination | 41° 12′ 56.17″[2] |
Characteristics | |
Evolutionary stage | M supergiant[1] |
Spectral type | M0I-M7I[1] |
Variable type | Luminous Red Nova |
Details | |
Radius | 2,000[3] R☉ |
Luminosity | 900,000[3][a] L☉ |
Temperature | 4,000[3] K |
Other designations | |
M31 V1006, M31 V1007, McD 88 1 | |
Database references | |
SIMBAD | data |
M31-RV is a possible red cataclysmic variable star located in the Andromeda Galaxy (M31) that experienced an outburst in 1988, which is similar to the outburst V838 Monocerotis experienced in 2002.[3] Such objects have been called luminous red novae or intermediate-luminosity red transients. During the outburst, both V838 Mon and M31-RV reached a maximum absolute visual magnitude of -9.8.[1]
In 2006, the area around M31-RV was observed using the Hubble Space Telescope, but only red giants were seen. Most likely the star either became too dim for Hubble to see, the star is a companion of one of the red giants, or the star is one of the red giants themselves.[2]
M31-RV reached a peak visual magnitude of 17 before fading rapidly and showing dust formation. The most likely explanation states that these outbursts occur during stellar merger events.[4]
arxiv1
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