Location of 41 Sex on the map (circled) | |
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
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Constellation | Sextans |
Right ascension | 10 50 18.05639 |
Declination | −08° 53′ 51.9538″ |
Apparent magnitude (V) | 5.79±0.01 |
Characteristics | |
Aa | |
Spectral type | kA3 hA7V mA9 |
U−B color index | +0.13 |
B−V color index | +0.16 |
Ab | |
Spectral type | F/G |
Astrometry | |
Radial velocity (Rv) | −4.9±2.9 km/s |
Proper motion (μ) | RA: −5.694 mas/yr Dec.: −15.814 mas/yr |
Parallax (π) | 10.5160 ± 0.0428 mas |
Distance | 310 ± 1 ly (95.1 ± 0.4 pc) |
Absolute magnitude (MV) | +0.91 |
Orbit | |
Primary | Aa |
Period (P) | 6.1670 d |
Eccentricity (e) | 0.014±0.006 |
Periastron epoch (T) | 2,453,690.7442±0.0011 JD |
Argument of periastron (ω) (secondary) | 272±4° |
Semi-amplitude (K1) (primary) | 46.67±0.04 km/s |
Semi-amplitude (K2) (secondary) | 93.06±0.20 km/s |
Details | |
Aa | |
Mass | 2.23 M☉ |
Radius | 3.10±0.16 R☉ |
Luminosity | 32.6±1.7 L☉ |
Surface gravity (log g) | 3.83 −0.07 cgs |
Temperature | 7,759 K |
Metallicity | −0.23 dex |
Rotational velocity (v sin i) | 24 km/s |
Age | 698 −108 Myr |
Ab | |
Mass | 1.05 M☉ |
Radius | 1.3±0.2 R☉ |
Luminosity | 1.8±0.5 L☉ |
Rotational velocity (v sin i) | 10 km/s |
Other designations | |
41 Sex, 74 G. Sextantis[15], BD−08°3018, FK5 1281, GC 14906, HD 93903, HIP 52980, HR 4237, SAO 137823, CCDM J10503-0853A, WDS J10503-0854A | |
Database references | |
SIMBAD | data |
41 Sextantis (HD 93903; HR 4237; 74 G. Sextantis), or simply 41 Sex is a spectroscopic binary located in the equatorial constellation Sextans. It has an apparent magnitude of 5.79, making it faintly visible to the naked eye under ideal conditions. The system is located relatively close at a distance of 310 light-years based on Gaia DR3 parallax measurements and it is drifting closer with a heliocentric radial velocity of approximately −4.9 km/s. At its current distance, 41 Sex's brightness is diminished by an interstellar extinction of 0.16 magnitudes and it has an absolute magnitude of +0.91.
The visible component has a stellar classification of kA3hA7VmA9, indicating that it is an Am star with the calcium K-lines of an A3 star, the hydrogen lines and effective temperature of an A7 main-sequence star, and the metal lines of an A9 star. Houk & Swift (1999) give a class of A2/3 III, indicating that it is an A-type star that has the characteristics of an A2 and A3 giant star. It has 2.23 times the mass of the Sun and a slightly enlarged radius 3.10 times that of the Sun. It radiates 32.6 times the luminosity of the Sun from its photosphere at an effective temperature of 7,759 K, giving it a white-hue when viewed in the night sky. 41 Sextantis Aa is metal-deficient with an iron abundance 58.9% that of the Sun and it spins modestly with a projected rotational velocity of 24 km/s.
The companion's spectrum is very weak compared to the primary, but it is said to be either a late F-type star or an early G-type star. It has 105% the mass of the Sun and 1.3 times the radius of the Sun. It radiates 1.8 times the luminosity of the Sun from its photosphere. It spins slowly with a projected rotational velocity of 10 km/s.
References
- ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27 – L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361. S2CID 17128864.
- ^ Abt, Helmut A.; Morrell, Nidia I. (July 1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182. ISSN 0067-0049. S2CID 120495962.
- ^ Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
- ^ Fekel, Francis C.; Williamson, Michael H. (November 1, 2010). "New Precision Orbits of Bright Double-lined Spectroscopic Binaries. V. The Am Stars HD 434 and 41 Sextantis". The Astronomical Journal. 140 (5): 1381–1390. Bibcode:2010AJ....140.1381F. doi:10.1088/0004-6256/140/5/1381. ISSN 0004-6256. S2CID 14261237.
- ^ Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. eISSN 1562-6873. ISSN 1063-7737. S2CID 119231169.
- ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. eISSN 1562-6873. ISSN 1063-7737. S2CID 119257644.
- ^ Worek, Thaddeus F. (May 1998). "Concerning the Reported Phase‐modulated Changes in the Spectrum of 41 Sextantis". Publications of the Astronomical Society of the Pacific. 110 (747): 580–585. Bibcode:1998PASP..110..580W. doi:10.1086/316160. ISSN 0004-6280. S2CID 121074533.
- ^ Kraicheva, Z.; Popova, E.; Tutukov, A.; Yungelson, L. (July 1980). "Catalogue of physical parameters of spectroscopic binary stars". Bull. Inf. Centre Données Stellaires. 19: 71. Bibcode:1980BICDS..19...71K. S2CID 118298938.
- ^ Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (April 8, 2004). "The angular sizes of dwarf stars and subgiants: Surface brightness relations calibrated by interferometry". Astronomy & Astrophysics. 426 (1): 297–307. arXiv:astro-ph/0404180. Bibcode:2004A&A...426..297K. doi:10.1051/0004-6361:20035930. eISSN 1432-0746. ISSN 0004-6361. S2CID 6077801.
- ^ McDonald, I.; Zijlstra, A. A.; Watson, R. A. (15 June 2017). "Fundamental parameters and infrared excesses of Tycho–Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770–791. arXiv:1706.02208. Bibcode:2017MNRAS.471..770M. doi:10.1093/mnras/stx1433. eISSN 1365-2966. ISSN 0035-8711. S2CID 73594365.
- Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. eISSN 1538-3881. hdl:1721.1/124721. S2CID 166227927.
- ^ Kunzli, M.; North, P. (February 1998). "Behaviour of calcium abundance in Am-Fm stars with evolution". Astronomy and Astrophysics. 330: 651–658. arXiv:astro-ph/9710223. Bibcode:1998A&A...330..651K. doi:10.48550/ARXIV.ASTRO-PH/9710223. S2CID 5679821.
- ^ Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. eISSN 1432-0746. ISSN 0004-6361. S2CID 131780028.
- Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode:1879RNAO....1.....G.
- "* 41 Sex". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved April 12, 2024.
- Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017). "Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars". Monthly Notices of the Royal Astronomical Society. 472 (4): 3805–3820. arXiv:1709.01160. Bibcode:2017MNRAS.472.3805G. doi:10.1093/mnras/stx2219. eISSN 1365-2966. ISSN 0035-8711. S2CID 118879856.
- Houk, Nancy; Swift, Carrie (1999). Michigan catalogue of two-dimensional spectral types for the HD Stars. Vol. 5. Bibcode:1999mctd.book.....H.
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