Astronomy:R Monocerotis

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Short description: Variable star in the constellation Monoceros
R Monocerotis
Ngc2261.jpg
R Monocerotis is at the bottom left of this photo.
Credit: HST/NASA/JPL
Observation data
Equinox J2000.0]] (ICRS)
Constellation Monoceros
Right ascension  06h 39m 09.954s[1]
Declination +08° 44′ 09.56″[1]
Apparent magnitude (V) 11.85[2]
Characteristics
Spectral type B8IIIev[3]
Variable type T Tauri[2]
Astrometry
Distance2600 ly
(800[4] pc)
Details
Mass~2–10[5] M
Age~105 yr[5] years
Other designations
R Mon, BD+08°1427, 2MASS J06390995+0844097, NGC 2261[2]
Database references
SIMBADdata

R Monocerotis, abbreviated R Mon, is a very young binary star[5] system in the equatorial constellation of Monoceros. The apparent magnitude of R Mon varies between 10 and 12 and the spectral type is B8IIIe.[3]

A visual band light curve for R Monocerotis, plotted from ASAS data[6]

This is a massive Herbig Ae/Be star, a type of pre-main-sequence star that is surrounded by an orbiting circumstellar disk of gas and dust. This disk has a mass of ~0.007 M and extends outward to a distance of under 150 astronomical unit|AU from the host. Because of this dust, the star is obscured from direct visual sight but can still be observed in the infrared.[5] R Mon is still in the accretion phase of star formation and it is driving an optically opaque bipolar outflow with a velocity of 9 km/s. The northern flow is blue-shifted, and thus moving more toward the Sun.[7] There is a T Tauri-type stellar companion at an angular separation of 0.69 from the primary.[5]

This system is located in a diffuse nebula called "Hubble's Variable Nebula" (NGC 2261), which is being illuminated by a conical beam of light from the primary.[5]

References

  1. 1.0 1.1 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. 2.0 2.1 2.2 "R Mon". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=R+Mon. 
  3. 3.0 3.1 Mora, A. et al. (2001). "EXPORT: Spectral classification and projected rotational velocities of Vega-type and pre-main sequence stars". Astronomy and Astrophysics 378: 116–131. doi:10.1051/0004-6361:20011098. Bibcode2001A&A...378..116M. 
  4. Manoj, P. (2006). "Evolution of Emission-Line Activity in Intermediate-Mass Young Stars". The Astrophysical Journal 653 (1): 657–674. doi:10.1086/508764. Bibcode2006ApJ...653..657M. 
  5. 5.0 5.1 5.2 5.3 5.4 5.5 Fuente, A. et al. (October 2006). "A Keplerian Gaseous Disk around the B0 Star R Monocerotis". The Astrophysical Journal 649 (2): L119–L122. doi:10.1086/508349. Bibcode2006ApJ...649L.119F. 
  6. "ASAS All Star Catalogue". The All Sky Automated Survey. http://www.astrouw.edu.pl/asas/?page=aasc. 
  7. Sandell, Göran et al. (February 2020). "The Molecular Outflow from R Mon". The Astrophysical Journal 889 (2): 9. doi:10.3847/1538-4357/ab6593. 138. Bibcode2020ApJ...889..138S. 

Further reading

External links