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BF Orionis

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Young protostar system
BF Orionis

A visual band light curve For BF Orionis, adapted from Grinin et al. (2010)
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05 37 13.2624
Declination −06° 35′ 00.5654″
Apparent magnitude (V) 9.69
Characteristics
Evolutionary stage Herbig Ae/Be star
Spectral type A5II-III
Apparent magnitude (g) 10.38
Astrometry
Proper motion (μ) RA: 0.873±0.025 mas/yr
Dec.: 0.654±0.023 mas/yr
Parallax (π)2.6173 ± 0.0279 mas
Distance1,250 ± 10 ly
(382 ± 4 pc)
Details
Mass1.85
−0.00 M
Radius1.59±0.20 R
Luminosity39 L
Surface gravity (log g)3.5 cgs
Temperature8750 K
Rotational velocity (v sin i)37±2 km/s
Age17.14
−0.00 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.

Properties

BF Orionis is a Herbig Ae/Be star variable similar to UX Orionis. It is still accreting mass, producing about 2L through the release of gravitational energy, and is surrounded by a massive, optically thick protoplanetary disk of 0.005±0.002M visible nearly edge-on. The brightness of the star is strongly variable, with irregular deep minima down to 13th magnitude. The variations are suspected to be partly caused by a brown dwarf or massive planet embedded in the protoplanetary disk, together with very large comets.

Unlike typical Herbig Ae/Be stars, 90-95% of which do not have detectable magnetic fields, BF Orionis has a fairly strong longitudinal magnetic field of −144±21 gauss. It also has small (0.11 magnitude) short-period, single-mode pulsations of the Delta Scuti type.

References

  1. ^ Grinin, V. P.; Rostopchina, A. N.; Barsunova, O. Yu.; Demidova, T. V. (2010). "Mechanism for cyclical activity of the Herbig Ae star BF Ori". Astrophysics. 53 (3): 367–372. Bibcode:2010Ap.....53..367G. doi:10.1007/s10511-010-9128-7. S2CID 56017726.
  2. ^ 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.
  3. ^ Wade, G. A.; Bagnulo, S.; Drouin, D.; Landstreet, J. D.; Monin, D. (2007). "A search for strong, ordered magnetic fields in Herbig Ae/Be stars". Monthly Notices of the Royal Astronomical Society. 376 (3): 1145–1161. arXiv:astro-ph/0701387. Bibcode:2007MNRAS.376.1145W. doi:10.1111/j.1365-2966.2007.11495.x. S2CID 14156014.
  4. ^ 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. ^ 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.
  8. Shevchenko, V. S.; Ezhkova, O. V. (2001). "Long-Term Cyclicity of the Herbig Ae Star BF Ori: Giant Protocomets and Accretion from a Protoplanetary Disk". Astronomy Letters. 27 (1): 39. Bibcode:2001AstL...27...39S. doi:10.1134/1.1336861. S2CID 121443217.
  9. Marconi, M.; Ripepi, V.; Alcala', J. M.; Covino, E.; Palla, F.; Terranegra, L. (2000). "Pulsation in two Herbig Ae stars: HD 35929 and V351 Ori". Astronomy and Astrophysics. 355. arXiv:astro-ph/0002466. Bibcode:2000A&A...355L..35M.
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