NO Aurigae
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 05h 40m 42.050s[1] |
Declination | +31° 55′ 14.20″[1] |
Apparent magnitude (V) | 6.21[2] (6.06 - 6.44[3]) |
Characteristics | |
Evolutionary stage | Asymptotic giant branch[4] |
Spectral type | M2S Iab[3] |
U−B color index | +2.22[5] |
B−V color index | +2.09[5] |
R−I color index | +1.41[5] |
Variable type | LC[3] |
Absolute magnitude (MV) | −5.88[2] |
Details | |
Mass | 4.93[7] M☉ |
Radius | 269[8] R☉ |
Luminosity | 9,075[8] L☉ |
Surface gravity (log g) | −0.037[8] cgs |
Temperature | 3,435[8] K |
58322 | |
Database references | |
SIMBAD | data |
Data sources: | |
NO Aurigae is a pulsating
light years
away.
Variability
NO Aurigae is listed in the General Catalogue of Variable Stars as a slow irregular variable, indicating that no regularity could be found in the brightness variations. Other studies have suggested possible periods of 102.1, 173, and 226 days, and would classify it as a semiregular variable star.[10] The maximum visual magnitude range is 6.05–6.50.[10]
Properties
Most studies of NO Aurigae treat it as a red supergiant member of the Auriga OB1 stellar association at about 1.4 kpc.[11][12] On this basis it would have a luminosity around 67,000 L☉ and a radius around 630 R☉.[2][11]
NO Aurigae is an
Asymptotic Giant Branch stars which can appear with supergiant spectra due to their large size and low mass.[4] Possible detection of Technetium in the spectrum is a symptom of the third dredge-up which occurs only in late AGB stars.[12]
References
- ^ .
- ^ S2CID 15109583.
- ^ Bibcode:2009yCat....102025S.
- ^ S2CID 14294870.
- ^ Bibcode:2002yCat.2237....0D.
- S2CID 17804304.
- S2CID 111387483.
- ^ S2CID 73594365.
- ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
- ^ Bibcode:2006SASS...25...47W.
- ^ S2CID 119276502.
- ^ S2CID 17789027.