11 Orionis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Orion |
| Right ascension | 05h 04m 34.14916s[1] |
| Declination | +15° 24′ 14.7771″[1] |
| Spectral type | B9 IV[2] |
11 Orionis (11 Ori) is a blue supergiant star in the constellation Orion. Its apparent magnitude is 4.66. It is a chemically peculiar star known as an Ap star, with enhanced Silicon and Chromium lines in its spectrum.[3]
References
- 1 2 Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ↑ Zorec, J.; Cidale, L.; Arias, M. L.; Frémat, Y.; Muratore, M. F.; Torres, A. F.; Martayan, C. (2009). "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff". Astronomy and Astrophysics 501: 297. arXiv:0903.5134. Bibcode:2009A&A...501..297Z. doi:10.1051/0004-6361/200811147.
- ↑ Stigler, Ch.; Maitzen, H. M.; Paunzen, E.; Netopil, M. (2014). "Spectrophotometric analysis of the 5200 Å region for peculiar and normal stars". Astronomy & Astrophysics 562: A65. arXiv:1402.1021. Bibcode:2014A&A...562A..65S. doi:10.1051/0004-6361/201322300.
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