AV Microscopii: Difference between revisions
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Citation bot (talk | contribs) Alter: template type. Add: issue, doi, s2cid, location. Removed parameters. Some additions/deletions were actually parameter name changes. | You can use this bot yourself. Report bugs here. | Suggested by Abductive | Category:Objects with variable star designations | via #UCB_Category |
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<ref name=GaiaDR2>{{Cite Gaia DR2|6678030179359993600}}</ref> |
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<ref name=houk1978>{{cite |
<ref name=houk1978>{{cite book |
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| last1=Houk | first1=Nancy |
| last1=Houk | first1=Nancy |
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| title=Michigan catalogue of two-dimensional spectral types for the HD stars |
| title=Michigan catalogue of two-dimensional spectral types for the HD stars |
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| volume=2 | |
| volume=2 | location=Ann Arbor |
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| publisher=Dept. of Astronomy, University of Michigan |
| publisher=Dept. of Astronomy, University of Michigan |
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| year=1978 | bibcode=1978mcts.book.....H |
| year=1978 | bibcode=1978mcts.book.....H }}</ref> |
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<ref name=Anderson2012>{{cite journal |
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| volume=38 | issue=5 | pages=331 | year=2012 |
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| bibcode=2012AstL...38..331A | arxiv=1108.4971 |
| bibcode=2012AstL...38..331A | arxiv=1108.4971 |
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| doi=10.1134/S1063773712050015 }}</ref> |
| doi=10.1134/S1063773712050015 | s2cid=119257644 }}</ref> |
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<ref name=AAVSOAV>{{cite web |
<ref name=AAVSOAV>{{cite web |
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| volume=400 | issue=4 | pages=1945–1961 |date=December 2009 |
| volume=400 | issue=4 | pages=1945–1961 |date=December 2009 |
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| bibcode=2009MNRAS.400.1945T | arxiv=0908.3228 |
| bibcode=2009MNRAS.400.1945T | arxiv=0908.3228 |
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| doi=10.1111/j.1365-2966.2009.15588.x }}</ref> |
| doi=10.1111/j.1365-2966.2009.15588.x | s2cid=15358380 }}</ref> |
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<ref name=Samus2017>{{cite journal |
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| version=5.1 | journal=Astronomy Reports |
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| year=2017 | volume=61 | issue=1 | pages=80–88 |
| year=2017 | volume=61 | issue=1 | pages=80–88 |
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| bibcode=2017ARep...61...80S }}</ref> |
| doi=10.1134/S1063772917010085 | bibcode=2017ARep...61...80S | s2cid=125853869 }}</ref> |
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<ref name=Evans1959>{{cite journal |
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| journal=Monthly Notices of the Royal Astronomical Society |
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| volume=119 | page=638 | date=1959 |
| volume=119 | page=638 | date=1959 |
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| doi=10.1093/mnras/119.6.638 | bibcode=1959MNRAS.119..638E | doi-access=free }}</ref> |
| issue=6 | doi=10.1093/mnras/119.6.638 | bibcode=1959MNRAS.119..638E | doi-access=free }}</ref> |
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<ref name=Eggen1976>{{cite journal |
<ref name=Eggen1976>{{cite journal |
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Revision as of 10:37, 8 October 2020
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Microscopium |
| Right ascension | 20h 41m 24.66513s[1] |
| Declination | −42° 08′ 01.6196″[1] |
| Apparent magnitude (V) | 6.28[2] (6.25 – 6.35)[3] |
| Characteristics | |
| Spectral type | M4 III[4] |
| B−V color index | 1.584±0.019[2] |
| Variable type | LC:[3] |
| Astrometry | |
| Radial velocity (Rv) | −22.9±0.9[2] km/s |
| Proper motion (μ) | RA: +46.627[1] mas/yr Dec.: −32.891[1] mas/yr |
| Parallax (π) | 4.3815 ± 0.1715 mas[1] |
| Distance | 740 ± 30 ly (228 ± 9 pc) |
| Absolute magnitude (MV) | −1.40[2] |
| Details | |
| Radius | 77.5+3.2 −16.4[1] R☉ |
| Luminosity | 849±38[1] L☉ |
| Temperature | 3,539+448 −70[1] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
AV Microscopii is a variable star in the southern constellation of Microscopium. It is a dim, red-hued star near the lower limit of visibility to the naked eye with a baseline apparent visual magnitude of 6.28.[2] The star is located approximately 740 light years away from the Sun, based on parallax,[1] but is moving closer with a radial velocity of −23 km/s.[2] It is a member of the Milky Way's old disk population.[6]
Based upon a stellar classification of M4 III,[4] this is an aging red giant star,[4] having exhausted the supply of hydrogen at its core then expanded to around 78[1] times the Sun's radius. Earlier it had been classed as M3 II,[7] with the luminosity class of a bright giant. Samus et al. (2017) have it tentatively classified as an irregular variable of subtype LC, suggesting this is a supergiant star.[3] It is a pulsating variable with multiple periods discovered,[8] ranging in apparent visual magnitude between 6.25 and 6.35.[3][9] The star radiates 849 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,539 K.[1]
| Period (days) | 22.3 | 23.3 | 30.3 | 31.0 | 32.3 | 45.0 | 110.7 |
| Amplitude (mag.) | 0.038 | 0.050 | 0.017 | 0.027 | 0.019 | 0.025 | 0.018 |
References
- ^ a b c d e f g h i j k Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d e f Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.
- ^ a b c d Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
- ^ a b c Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 2. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
- ^ "AV Mic". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-11.
- ^ Eggen, O. J. (August 1976). "A sample of old-disk-population red giants". Publications of the Astronomical Society of the Pacific. 88: 426–443. Bibcode:1976PASP...88..426E. doi:10.1086/129965.
- ^ Evans, David S.; et al. (1959). "Fundamental data for southern stars (Second List)". Monthly Notices of the Royal Astronomical Society. 119 (6): 638. Bibcode:1959MNRAS.119..638E. doi:10.1093/mnras/119.6.638.
- ^ a b Tabur, V.; et al. (December 2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society. 400 (4): 1945–1961. arXiv:0908.3228. Bibcode:2009MNRAS.400.1945T. doi:10.1111/j.1365-2966.2009.15588.x. S2CID 15358380.
- ^ Watson, Christopher (28 September 2009). "AV Microscopii". AAVSO Website. American Association of Variable Star Observers. Retrieved 20 March 2015.
