 A white light light curve for UY Sextantis, adapted from Billeres et al. (1997).[1] All five panels form a single 10,000 second light curve, with the top panel continued on the second panel, etc. | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Sextans |
| Right ascension | 10h 50m 02.826s[2] |
| Declination | −00° 00′ 36.88″[2] |
| Apparent magnitude (V) | 13.47 |
| Characteristics | |
| Spectral type | sdO9VII:He6[3] |
| Variable type | V361 Hya[1] |
| Astrometry | |
| Radial velocity (Rv) | 13.6[4] km/s |
| Proper motion (μ) | RA: −20.528 mas/yr[2] Dec.: −38.421 mas/yr[2] |
| Parallax (π) | 1.4559 ± 0.0789 mas[2] |
| Distance | 2,200 ± 100 ly (690 ± 40 pc) |
| Details | |
| Mass | 0.490±0.014[5] M☉ |
| Radius | 0.17±0.01[5] R☉ |
| Luminosity | 25.86+3.28 −2.61[5] L☉ |
| Surface gravity (log g) | 5.83±0.01[4] cgs |
| Temperature | 34,850±90[4] K |
| Rotation | 24.6±3.5 d[5] |
| Other designations | |
| Database references | |
| SIMBAD | data |
PG 1047+003 is a post-AGB blue-white subdwarf star, located in the constellation of Sextans. The star is classed as member of the V361 Hydrae type (or also called sdBVr type) class of pulsators in the field of asteroseismology.[1] No additional stellar companion has been detected in tight orbit or imaged around the subdwarf star.[7]
YouTube Encyclopedic
-
1/4Views:1 693 02952 4261 4512 028
-
MULTIPLICAÇÃO (números decimais) - Aula 05
-
1日100言ーリクエストにお答えしてー英語英会話一日一言001〜100
-
Previous year solutions DU 2016 (DU 2016 Physical Part 1)
-
MABA SENAI - PROVA DE 2019 - QUESTÃO 27 - POLÍGONO REGULAR E SEUS ÂNGULOS
Transcription
References
- ^ a b c Billeres; et al. (1997). "Discovery of p-mode Instabilities in the Hot Subdwarf B Star PG 1047+003". Astrophysical Journal Letters. 487 (1): 81–84. Bibcode:1997ApJ...487L..81B. doi:10.1086/310882.
- ^ a b c d 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.
- ^ Drilling, J. S.; et al. (2013). "An MK-like system of spectral classification for hot subdwarfs". Astronomy & Astrophysics. 551: A31. Bibcode:2013A&A...551A..31D. doi:10.1051/0004-6361/201219433.
- ^ a b c Lei, Zhenxin; et al. (November 2018). "New Hot Subdwarf Stars Identified in Gaia DR2 with LAMOST DR5 Spectra". The Astrophysical Journal. 868 (1): 9. arXiv:1810.09625. Bibcode:2018ApJ...868...70L. doi:10.3847/1538-4357/aae82b. S2CID 250892206. 70.
- ^ a b c d Reed, M. D.; et al. (March 2020). "K2 observations of the pulsating subdwarf B stars UY Sex and V1405 Ori". Monthly Notices of the Royal Astronomical Society. 492 (4): 5202–5217. Bibcode:2020MNRAS.492.5202R. doi:10.1093/mnras/staa144.
- ^ "UY Sex". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2022-01-26.
{{cite web}}: CS1 maint: postscript (link) - ^ O'Donoghue; Koen; Lynas-Gray; Kilkenny; Van Wyk (1998). "The EC14026 stars - VI. PG1047+003". Monthly Notices of the Royal Astronomical Society. 296 (2): 306–316. Bibcode:1998MNRAS.296..306O. doi:10.1046/j.1365-8711.1998.01311.x.
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
| Galaxies |
| ||||||||||||
| |||||||||||||
 | This variable star–related article is a stub. You can help Wikipedia by expanding it. |
This page was last edited on 27 March 2024, at 17:24