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41 Sextantis

[edit]
41 Sextantis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Sextans
Right ascension 10h 50m 18.05639s[1]
Declination −08° 53′ 51.9538″[1]
Apparent magnitude (V) 5.79±0.01[2]
Characteristics
Aa
Spectral type kA3 hA7V mA9[3]
U−B color index +0.13[4]
B−V color index +0.16[4]
Ab
Spectral type F/G[5]
Astrometry
Radial velocity (Rv)−4.9±2.9[6] km/s
Proper motion (μ) RA: −5.694 mas/yr[1]
Dec.: −15.814 mas/yr[1]
Parallax (π)10.5160 ± 0.0428 mas[1]
Distance310 ± 1 ly
(95.1 ± 0.4 pc)
Absolute magnitude (MV)+0.91[7]
Orbit[5]
PrimaryAa
Period (P)6.1670 d
Eccentricity (e)0.014±0.006[8]
Periastron epoch (T)2,453,690.7442±0.0011 JD
Argument of periastron (ω)
(secondary)		272±4[8]°
Semi-amplitude (K1)
(primary)		46.67±0.04 km/s
Semi-amplitude (K2)
(secondary)		93.06±0.20 km/s
Details
Aa
Mass2.23[9] M☉
Radius3.10±0.16[10] R☉
Luminosity32.6±1.7[11] L☉
Surface gravity (log g)3.83+0.10
−0.07[12] cgs
Temperature7,759[13] K
Metallicity [Fe/H]−0.23[14] dex
Rotational velocity (v sin i)24[5] km/s
Age698+128
−108[13] Myr
Ab
Mass1.05[9] M☉
Radius1.3±0.2[5] R☉
Luminosity1.8±0.5[5] L☉
Rotational velocity (v sin i)10[5] 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[16]
Database references
SIMBADdata

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,[2] 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[1] and it is drifting closer with a heliocentric radial velocity of approximately −4.9 km/s.[6] At its current distance, 41 Sex's brightness is diminished by an interstellar extinction of 0.16 magnitudes[17] and it has an absolute magnitude of +0.91.[7]

The visible component has a stellar classification of kA3hA7VmA9,[3] 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. It has 2.23 times the mass of the Sun[9] and a slightly enlarged radius 3.10 times that of the Sun.[10] It radiates 32.6 times the luminosity of the Sun[11] from its photosphere at an effective temperature of 7,759 K,[13] 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[14] and it spins modestly with a projected rotational velocity of 24 km/s.[5]

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.[5] It has 105% the mass of the Sun[9] and 1.3 times the radius of the Sun.[5] It radiates 1.8 times the luminosity of the Sun from its photosphere.[5] It spins slowly with a projected rotational velocity of 10 km/s.[5]


References

[edit]
  1. ^ a b c d e 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.
  2. ^ a b 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.
  3. ^ a b 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.
  4. ^ a b 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.
  5. ^ a b c d e f g h i j k 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.
  6. ^ a b 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.
  7. ^ a b 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.
  8. ^ a b 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.
  9. ^ a b c d 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.
  10. ^ a b 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.
  11. ^ a b 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.
  12. ^ 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.
  13. ^ a b c 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.
  14. ^ a b 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.
  15. ^ 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.
  16. ^ "* 41 Sex". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved April 12, 2024.
  17. ^ 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.
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S Equueli

[edit]
S Equulei
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Equuleus
Right ascension 20h 57m 12.84053s[1]
Declination +05° 04′ 49.4257″[1]
Apparent magnitude (V) 8.35 - 10.40[2]
Characteristics
Spectral type B8-9.5 V + F9 III-IV[3]
Variable type Algol variable[4]
Astrometry
Radial velocity (Rv)−48.0±7.4[5] km/s
Proper motion (μ) RA: +16.889 mas/yr[1]
Dec.: −4.740 mas/yr[1]
Parallax (π)2.4961 ± 0.0281 mas[1]
Distance1,310 ± 10 ly
(401 ± 5 pc)
A
Absolute bolometric
magnitude (Mbol)		−0.49[6]
B
Absolute bolometric
magnitude (Mbol)		+3.36[6]
Orbit[7]
Period (P)3.4361 d
Semi-major axis (a)13.70 R☉
Eccentricity (e)0.145±0.029
Inclination (i)89.0±1.2°
Periastron epoch (T)2,437,968.3230 JD
Argument of periastron (ω)
(secondary)		83.6±14.9°
Semi-amplitude (K1)
(primary)		23.4±0.8 km/s
Details
A
Mass3.19[8] M☉
Radius2.74±0.09[3] R☉
Luminosity105+27
−22[3] L☉
Surface gravity (log g)4.07±0.01[3] cgs
Temperature12,189[8] K
Rotational velocity (v sin i)52.4±4.4 km/s
B
Mass0.42[8] M☉
Radius3.24±0.10[3] R☉
Luminosity7.24+1.88
−1.49[3] L☉
Surface gravity (log g)3.04±0.01[3] cgs
Temperature5,794[8] K


References

[edit]
  1. ^ a b c d 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.
  2. ^ Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. eISSN 1562-6881. ISSN 1063-7729. S2CID 125853869.
  3. ^ a b c d e f g Soydugan, F.; Frasca, A.; Soydugan, E.; Catalano, S.; Demircan, O.; Ibanoglu, C. (August 21, 2007). "A spectroscopic study of the Algol-type binaries S Equulei and KO Aquilae: absolute parameters and mass transfer". Monthly Notices of the Royal Astronomical Society. 379 (4): 1533–1545. arXiv:0706.3835. Bibcode:2007MNRAS.379.1533S. doi:10.1111/j.1365-2966.2007.12065.x. ISSN 0035-8711.
  4. ^ Mallama, A. D. (October 1980). "New ephemerides for 120 eclipsing binary stars". The Astrophysical Journal Supplement Series. 44: 241. Bibcode:1980ApJS...44..241M. doi:10.1086/190693. ISSN 0067-0049. S2CID 121834691.
  5. ^ Kharchenko, N.V.; Scholz, R.-D.; Piskunov, A.E.; Röser, S.; Schilbach, E. (November 2007). "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations". Astronomische Nachrichten. 328 (9): 889–896. arXiv:0705.0878. Bibcode:2007AN....328..889K. doi:10.1002/asna.200710776. eISSN 1521-3994. ISSN 0004-6337. S2CID 119323941.
  6. ^ a b Surkova, L. P.; Svechnikov, M. A. (January 2004). "VizieR Online Data Catalog: Semi-detached eclipsing binaries (Surkova+, 2004)". VizieR Online Data Catalog. 5115. Bibcode:2004yCat.5115....0S.
  7. ^ Plavec, M. (1966). "S Equulei, a new close binary with gaseous streams". Bulletin of the Astronomical Institutes of Czechoslovakia. 17: 295. Bibcode:1966BAICz..17..295P. ISSN 0004-6248. S2CID 231164853.
  8. ^ a b c d Soydugan, F.; Frasca, A.; Catalano, S.; Ibanoǧlu, C.; Demircan, O.; Soydugan, E. (March 2005). "A spectroscopic study of some Algol systems". Proceedings of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. 560: 975. Bibcode:2005ESASP.560..975S.
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