BF Orionis

BF Orionis

A visual band light curve For BF Orionis, adapted from Grinin et al. (2010)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 37m 13.2624s[2]
Declination −06° 35′ 00.5654″[2]
Apparent magnitude (V) 9.69
Characteristics
Evolutionary stage Herbig Ae/Be star
Spectral type A5II-III[3]
Apparent magnitude (g) 10.38
Astrometry
Proper motion (μ) RA: 0.873±0.025 mas/yr[2]
Dec.: 0.654±0.023 mas/yr[2]
Parallax (π)2.6173 ± 0.0279 mas[2]
Distance1,250 ± 10 ly
(382 ± 4 pc)
Details
Mass1.85+0.15
−0.00
[4] M
Radius1.59±0.20[4] R
Luminosity39[5] L
Surface gravity (log g)3.5[6] cgs
Temperature8750[6] K
Rotational velocity (v sin i)37±2[3] km/s
Age17.14+2.80
−0.00
[4] Myr
Other designations
BD-06 1259, GSC 04778-01087, HIP 26403, 2MASS J05371326-0635005, Gaia DR2 3016930993175537536, Gaia EDR3 3016930993175889792, TYC 4778-1087-1
Database references
SIMBADdata

BF Orionis is a young Herbig Ae/Be star in the constellation of Orion about 1250 light years away, within the Orion Nebula. It is the most massive star of the small birth cluster of four stars.[7]

  1. ^ Cite error: The named reference Grinin2010 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference EDR3 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Wade2007 was invoked but never defined (see the help page).
  4. ^ a b c Guzmán-Díaz, J.; Mendigutía, I.; Montesinos, B.; Oudmaijer, R. D.; Vioque, M.; Rodrigo, C.; Solano, E.; Meeus, G.; Marcos-Arenal, P. (2021), "Homogeneous study of Herbig Ae/Be stars from spectral energy distributions and Gaia EDR3", Astronomy & Astrophysics, 650: A182, arXiv:2104.11759, Bibcode:2021A&A...650A.182G, doi:10.1051/0004-6361/202039519, S2CID 233393918
  5. ^ Grinin, V. P.; Kozlova, O. V.; Natta, A.; Ilyin, I.; Tuominen, I.; Rostopchina, A. N.; Shakhovskoy, D. N. (2001). "Optical spectra of five UX Orionis-type stars". Astronomy and Astrophysics. 379 (2): 482. Bibcode:2001A&A...379..482G. doi:10.1051/0004-6361:20011280. S2CID 121844237.
  6. ^ a b Mora, A.; Eiroa, C.; Natta, A.; Grady, C. A.; De Winter, D.; Davies, J. K.; Ferlet, R.; Harris, A. W.; Miranda, L. F.; Montesinos, B.; Oudmaijer, R. D.; Palacios, J.; Quirrenbach, A.; Rauer, H.; Alberdi, A.; Cameron, A.; Deeg, H. J.; Garzón, F.; Horne, K.; Merín, B.; Penny, A.; Schneider, J.; Solano, E.; Tsapras, Y.; Wesselius, P. R. (2004). "Dynamics of the circumstellar gas in the Herbig Ae stars BF Orionis, SV Cephei, WW Vulpeculae and XY Persei". Astronomy & Astrophysics. 419: 225–240. arXiv:astro-ph/0402614. Bibcode:2004A&A...419..225M. doi:10.1051/0004-6361:20040096. S2CID 17149403.
  7. ^ Testi, L.; Palla, F.; Natta, A. (1998). "The onset of cluster formation around Herbig Ae/Be stars". arXiv:astro-ph/9811210.