S Monocerotis

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S Monocerotis
Monoceros constellation map.svg
S Monocerotis lies in NGC 2264 at the very northern edge of Monoceros.
Observation data
Epoch J2000       Equinox J2000
Constellation Monoceros
A
Right ascension 06h 40m 58.656s [1]
Declination +09° 53′ 44.71″ [1]
Apparent magnitude  (V)4.66 [2] (4.62 - 4.68 [3] ) + 5.90 [2]
B
Right ascension 06h 40m 58.566s [1]
Declination +09° 53′ 42.20″ [1]
Apparent magnitude  (V)7.830 [1]
Characteristics
Spectral type O7V((f))zvar [4] + O9.5Vn [5] + B2V [6]
U−B color index −1.034 [7]
B−V color index −0.261 [7]
Variable type Ia [3]
Astrometry
A
Radial velocity (Rv)22.00 [8]  km/s
Proper motion (μ)RA: −2.61 [9]   mas/yr
Dec.: −1.61 [9]   mas/yr
Parallax (π)3.55 ± 0.50  mas [9]
Distance 720 [5]   pc
Absolute magnitude  (MV)−5.21 [10]
B
Proper motion (μ)RA: −1.971 [11]   mas/yr
Dec.: −4.225 [11]   mas/yr
Parallax (π)1.4019 ± 0.0984  mas [11]
Distance 2,300 ± 200  ly
(710 ± 50  pc)
C
Proper motion (μ)RA: −1.464 [12]   mas/yr
Dec.: −2.746 [12]   mas/yr
Parallax (π)1.5438 ± 0.0394  mas [12]
Distance 2,110 ± 50  ly
(650 ± 20  pc)
Orbit [13]
PrimaryAa
CompanionAb
Period (P)108±12 yr
Semi-major axis (a)112.5±6  mas
Eccentricity (e)0.770+0.023
−0.030
Inclination (i)47±2°
Longitude of the node (Ω)60±3°
Periastron epoch (T)B 1996.05+0.15
−0.10
Argument of periastron (ω)
(secondary)		63±4°
Details
Aa
Mass 29.1 [2]   M☉
Radius 9.9 [14]   R☉
Luminosity 214,000 [14]   L☉
Surface gravity (log g)4.5 [15]   cgs
Temperature 38,500 [14]   K
Rotational velocity (v sin i)120 [16]  km/s
Ab
Mass 21.3 [2]   M☉
Age 3.1 [17]   Myr
Other designations
15 Monocerotis, HD 47839, HIP 31978, HR 2456, SAO 114258, BD+10°1220
Database references
SIMBAD data
ARICNS data
NGC 2264 including the Cone Nebula and the Christmas Tree Cluster (upside down in this image) with S Monocerotis at the very top of the image (and the base of the Christmas tree) NGC 2264 cluster.jpg
NGC 2264 including the Cone Nebula and the Christmas Tree Cluster (upside down in this image) with S Monocerotis at the very top of the image (and the base of the Christmas tree)

S Monocerotis, also known as 15 Monocerotis, is a massive multiple and variable star system located in the constellation Monoceros. It is the brightest star in the Christmas Tree open cluster in the area catalogued as NGC 2264.

S Monocerotis is found within an open cluster and the Washington Double Star Catalog lists many companion stars. [18] The closest and brightest is S Mon B, magnitude 7.8 and 3 arcseconds away. It is classified as B2 main sequence star with a mass of 7.31  M☉. Designated component C is an 11th-magnitude B8V star. [6] The cluster contains another dozen or so 9th and 10th magnitude stars and many fainter stars.

S Monocerotis A is a spectroscopic binary system with an eccentric orbit of about 112 years. [13] Since 1943, the spectrum of this star has served as the MK standard for O7 by which other stars are classified. [19] It is also an irregular variable star with a range of less than a tenth of a magnitude. The orbital parameters can be used to derive the masses of the two stars, giving 31 M☉ and 11 M☉. [6]

The distance to S Monocerotis and NGC 2264 has been derived in various ways, including dynamical parallax and isochrone fitting. These consistently give estimates of 700 - 900 parsecs, although this is double the likely distance derived from the Hipparcos parallax measurements. [9] Gaia Early Data Release 3 contains parallaxes for the companions components B and C of 1.4  mas and 1.5 mas respectively, consistent with the expected distance to the cluster.

Related Research Articles

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NGC 2346 is a planetary nebula near the celestial equator in the constellation of Monoceros, less than a degree to the ESE of Delta Monocerotis. It is informally known as the Butterfly Nebula. The nebula is bright and conspicuous with a visual magnitude of 9.6, and has been extensively studied. Among its most remarkable characteristics is its unusually cool central star, which is a spectroscopic binary, and its unusual shape.

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<span class="mw-page-title-main">R Monocerotis</span> Variable star in the constellation Monoceros

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<span class="mw-page-title-main">18 Monocerotis</span> Star in the constellation Monoceros

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<span class="mw-page-title-main">KQ Puppis</span> Binary star in the constellation Puppis

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<span class="mw-page-title-main">31 Cygni</span> Triple star system in the constellation Cygnus

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<span class="mw-page-title-main">CD Crucis</span> Eclipsing binary star system in the constellation Crux

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<span class="mw-page-title-main">HD 15558</span> Star in the constellation Cassiopeia

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<span class="mw-page-title-main">HD 151932</span> Star in the constellation of Scorpius

HD 151932, also known as WR 78, is a Wolf-Rayet star located in the constellation Scorpius, close to the galactic plane. Its distance is around 1,300 parsecs away from the Earth. Despite being a blue-colored Wolf-Rayet star, it is extremely reddened by interstellar extinction, so its apparent magnitude is brighter for longer-wavelength passbands. HD 151932 lies about 22′ west of the open cluster NGC 6231, the center of the OB association Scorpius OB1; it is not clear whether it is a part of the association or not. With an apparent magnitude of about 6.5, it is one of the few Wolf-Rayet stars that can be seen with the naked eye.

<span class="mw-page-title-main">HD 193322</span> Star group in the constellation Cygnus

HD 193322 is a group of six stars which appear to be at least loosely bound into a system in the constellation Cygnus. The stars comprise the core of the young open cluster Collinder 419, which contains a total of 51 known stars. Another prominent member of the cluster is the eclipsing binary star V470 Cygni. The cluster lies at a distance of about 3500 light years and its stars are only a few million years old.

<span class="mw-page-title-main">WR 120</span> Binary star system in the constellation Scutum

WR 120 is a binary containing two Wolf-Rayet stars in the constellation of Scutum, around 10,000 light years away. The primary is a hydrogen-free weak-lined WN7 star, the secondary is a hydrogen-free WN3 or 4 star, and the system is a possible member of the cluster Dolidze 33. From our point of view, WR 120 is reddened by 4.82 magnitudes, and it has the variable designation of V462 Scuti.

References

  1. 1 2 3 4 5 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode:2000A&A...355L..27H. doi:10.1888/0333750888/2862. ISBN   0333750888.
  2. 1 2 3 4 Cvetkovc, Zorica; Vince, Istvan; Ninkovic, Slobodan (2008). "Orbit of Binary 15 Monocerotis". arXiv: 0804.0698 [astro-ph].
  3. 1 2 Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  4. ↑ Sota, A.; Maíz Apellániz, J.; Walborn, N. R.; Alfaro, E. J.; Barbá, R. H.; Morrell, N. I.; Gamen, R. C.; Arias, J. I. (2011). "The Galactic O-Star Spectroscopic Survey. I. Classification System and Bright Northern Stars in the Blue-violet at R ~ 2500". The Astrophysical Journal Supplement. 193 (2): 24. arXiv: 1101.4002 . Bibcode:2011ApJS..193...24S. doi:10.1088/0067-0049/193/2/24. S2CID   119248206.
  5. 1 2 Cvetković, Z.; Vince, I.; Ninković, S. (2010). "A new orbit of binary 15 Monocerotis". New Astronomy. 15 (3): 302–306. Bibcode:2010NewA...15..302C. doi:10.1016/j.newast.2009.09.002.
  6. 1 2 3 Tokovinin, A. A. (1997). "MSC - a catalogue of physical multiple stars". Astronomy and Astrophysics Supplement Series. 124: 75–84. Bibcode:1997A&AS..124...75T. doi: 10.1051/aas:1997181 .
  7. 1 2 Oja, T. (August 1985). "Photoelectric photometry of stars near the north Galactic pole. II". Astronomy and Astrophysics Supplement Series. 61: 331–339. Bibcode:1985A&AS...61..331O.
  8. ↑ Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424 (2): 727–732. arXiv: astro-ph/0406573 . Bibcode:2004A&A...424..727P. doi:10.1051/0004-6361:20041213. S2CID   119387088.
  9. 1 2 3 4 Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv: 0708.1752 . Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID   18759600.
  10. ↑ Feinstein, A.; Vazquez, R. A.; Benvenuto, O. G. (1986). "Of-stars in young open clusters". Astronomy and Astrophysics. 159: 223. Bibcode:1986A&A...159..223F.
  11. 1 2 3 Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics . 649: A1. arXiv: 2012.01533 . Bibcode:2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657 . S2CID   227254300. (Erratum:  doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  12. 1 2 3 Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics . 649: A1. arXiv: 2012.01533 . Bibcode:2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657 . S2CID   227254300. (Erratum:  doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  13. 1 2 Maíz Apellániz, J. (2019). "Gaia DR2 distances to Collinder 419 and NGC 2264 and new astrometric orbits for HD 193 322 Aa,Ab and 15 Mon Aa,Ab". Astronomy and Astrophysics. 630: A119. arXiv: 1908.02040 . Bibcode:2019A&A...630A.119M. doi:10.1051/0004-6361/201935885. S2CID   247759810.
  14. 1 2 3 Herrero, A.; Kudritzki, R. P.; Vilchez, J. M.; Kunze, D.; Butler, K.; Haser, S. (1992). "Intrinsic parameters of galactic luminous OB stars". Astronomy and Astrophysics. 261: 209. Bibcode:1992A&A...261..209H.
  15. ↑ Sung, Hwankyung; Stauffer, John R.; Bessell, Michael S. (2009). "A Spitzer View of the Young Open Cluster NGC 2264". The Astronomical Journal. 138 (4): 1116–1136. arXiv: 0906.3072 . Bibcode:2009AJ....138.1116S. doi:10.1088/0004-6256/138/4/1116. S2CID   5272305.
  16. ↑ Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities". Contributi Osservatorio Astronomico di Padova in Asiago. 239 (1): 1. Bibcode:1970CoAsi.239....1B.
  17. ↑ Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (2010). "Masses and luminosities of O- and B-type stars and red supergiants". Astronomische Nachrichten. 331 (4): 349–360. arXiv: 1003.2335 . Bibcode:2010AN....331..349H. doi:10.1002/asna.200911355. S2CID   111387483.
  18. ↑ Worley, C. E.; Douglass, G. G. (1997). "The Washington Double Star Catalog (WDS, 1996.0)". Astronomy and Astrophysics Supplement Series. 125 (3): 523. Bibcode:1997A&AS..125..523W. doi: 10.1051/aas:1997239 .
  19. ↑ Garrison, R. F. (December 1993). "Anchor Points for the MK System of Spectral Classification". Bulletin of the American Astronomical Society. 25: 1319. Bibcode:1993AAS...183.1710G. Archived from the original on 2019-06-25. Retrieved 2012-02-04.
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