SX Arietis variable
SX Arietis variables are a class of variable stars. They are generally B-type main sequence stars of spectral types B0p to B9p— high-temperature analogues of Alpha2 Canum Venaticorum variables—and exhibit strong magnetic fields and intense He I and Si III spectral lines.[2] They have brightness fluctuations of approximately 0.1 magnitudes with periods of about one day. The prototype of this class is 56 Arietis, which bears the variable star designation SX Arietis.
List
The following list contains selected SX Arietis variable that are of interest to amateur or professional astronomy. Unless otherwise noted, the given magnitudes are in the V-band.
Star |
Average magnitude |
Spectral type |
Period (in days) |
Distance (in parsecs) |
---|---|---|---|---|
Alpha Sculptoris | 4.27 | B7IIIp | 238 | |
Sigma Lupi | 4.42 | B2III | 3.02 | 176 |
HD 125823 | 4.42 | B7IIIpv | 8.82 | 140 |
HR 2949 | 4.43 | B5IV | 1.90 | 113 |
28 Cygni | 4.93 | B2.5Ve | 0.70 | 317 |
36 Lyncis | 5.29 | B9 | 3.83 | 178 |
HD 142990 | 5.43 | B5V | 0.98 | 170 |
V692 Coronae Australis | 5.46 | B2.5III | 1.67 | 357 |
HD 21699 | 5.46 | B8IIImnp | 2.48 | 186 |
56 Arietis | 5.76 | B6IV-V | 0.73 | 154 |
HD 133880 | 5.79 | B8IVSi | 0.88 | 111 |
HD 28843 | 5.81 | B9III | 1.37 | 146 |
3 Scorpii | 5.87 | B8III/IV | 1.46 | 158 |
V957 Scorpii | 5.90 | B6V | 258 | |
V929 Scorpii | 5.92 | B8V | 1.49 | 161 |
HR 7355 | 6.02 | B2Vn | 0.52 | 273 |
HD 145792 | 6.42 | B6IV | 1.70 | 144 |
HD 37017 | 6.56 | B1.5V | [n 1] | 380 |
Sigma Orionis E | 6.61 | B2Vp | 1.19 | 329 |
HD 37776 | 6.96 | B2V | 1.54 | 330 |
HD 37058 | 7.30 | B3Vp | 15.26 | |
HD 184927 | 7.44 | B2V | 9.35 | 543 |
HD 191612 | 7.80 | O8fpe | 538 | 2041 |
HD 35298 | 7.91 | B7IV | 1.85 | 532 |
HD 36668 | 8.05 | B8V | 2.12 | 249 |
HD 34626 | 8.16 | B1.5IVnp | 0.50 | 483 |
Notes
- also an eclipsing binary
References
- Wraight, K. T.; Fossati, L.; Netopil, M.; Paunzen, E.; Rode-Paunzen, M.; Bewsher, D.; Norton, A. J.; White, Glenn J. (February 2012). "A photometric study of chemically peculiar stars with the STEREO satellites – I. Magnetic chemically peculiar stars". Monthly Notices of the Royal Astronomical Society. 420 (1): 757–772. doi:10.1111/j.1365-2966.2011.20090.x. Retrieved 26 October 2021.
- Good, Gerry A. (2012), Observing Variable Stars, The Patrick Moore Practical Astronomy Series, Springer Science & Business Media, p. 139, ISBN 9781447100553.
Samus N.N., Durlevich O.V., et al. Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.)
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.