Ross 248
| Data pengamatan Epos J2000 Ekuinoks J2000 | |
|---|---|
| Rasi bintang | Andromeda |
| Asensio rekta | 23j 41m 54.99d[1] |
| Deklinasi | +44° 10′ 40.8″[1] |
| Magnitudo tampak (V) | 12.29[2] |
| Ciri-ciri | |
| Kelas spektrum | M6e[3] |
| Indeks warna U−B | +1.48[2] |
| Indeks warna B−V | +1.92[2] |
| Jenis variabel | Flare star |
| Astrometri | |
| Kecepatan radial (Rv) | -81[4] km/s |
| Gerak diri (μ) | RA: 111[5] mdb/thn Dek.: -1584[5] mdb/thn |
| Paralaks (π) | 316,80±1,10[6] mdb |
| Jarak | 10,30 ± 0,04 tc (3,16 ± 0,01 pc) |
| Magnitudo mutlak (MV) | 14.79[7] |
| Detail | |
| Massa | 0.12[8] M☉ |
| Radius | 0.16[9] R☉ |
| Luminositas | 0.0018[10] L☉ |
| Gravitasi permukaan (log g) | 5.12[3] |
| Suhu | 2,799[3] K |
| Rotasi | v sin i < 3 km/s[11] |
| Penamaan lain | |
Ross 248 (HH Andromedae) adalah bintang katai merah yang terletak sejauh 10,3 tahun cahaya dari Bumi. Bintang ini berada di rasi bintang Andromeda.
Bintang ini memunyai 12% massa matahari, 16% jari-jari matahari, dan 0,2% luminositas matahari. Ross 248 merupakan bintang suar yang kadang-kadang luminositasnya meningkat.[12]
Referensi
- ^ a b Cutri, R. M.; et al. (2003). 2MASS All Sky Catalog of point sources. NASA/IPAC. Bibcode:2003tmc..book.....C.
- ^ a b c d "V* HH And – Flare Star". SIMBADa. Centre de Données astronomiques de Strasbourg. Diakses tanggal 2009-09-06.
- ^ a b c Cenarro, A. J.; Peletier, R. F.; Sánchez–blázquez, P.; Selam, S. O.; Toloba, E.; Cardiel, N.; Falcón–barroso, J.; Gorgas, J.; Jiménez-Vicente, J. (2007). "Medium-resolution Isaac Newton Telescope Library of Empirical Spectra – II. The Stellar Atmospheric Parameters". Monthly Notices of the Royal Astronomical Society. 374 (2): 664–690. doi:10.1111/j.1365-2966.2006.11196.x.
- ^ Wilson, Ralph Elmer (1953). General Catalogue of Stellar Radial Velocities. Washington: Carnegie Institution of Washington. Bibcode:1953QB901.W495.....
- ^ a b Lépine, Sébastien; Shara, Michael M (2005). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)". The Astronomical Journal. 129 (3): 1483–1522. doi:10.1086/427854.
- ^ Leggett, S. K. (1992). "Infrared colors of low-mass stars". Astrophysical Journal Supplement Series. 82 (1): 351–394. doi:10.1086/191720.
- ^ Schroeder, Daniel J.; Golimowski, David A.; Brukardt, Ryan A.; Burrows, Christopher J.; Caldwell, John J.; Fastie, William G.; Ford, Holland C.; Hesman, Brigette; Kletskin, Ilona (2000). "A Search for Faint Companions to Nearby Stars Using the Wide Field Planetary Camera 2". The Astronomical Journal. 119: 906–922. doi:10.1086/301227.
- ^ "The One Hundred Nearest Star Systems". Research Consortium on Nearby Stars. 2009-01-01. Diakses tanggal 2009-09-06.
- ^ Johnson, H. M.; Wright, C. D. (1983). "Predicted infrared brightness of stars within 25 parsecs of the Sun". Astrophysical Journal Supplement Series. 53: 643–711. doi:10.1086/190905. See p. 705.
- ^ West, Frederick R. (1999). "Monitoring Nearby Stars for Transits by Extrasolar Jovial Planets, II: Transits of M-Type (Red) Dwarf Stars by Close Extrasolar Giant (Jovian) Planets". The Journal of the American Association of Variable Star Observers. 27 (1): 77–78. Bibcode:1999JAVSO..27...77W.
- ^ Reiners, A.; Basri, G. (2007). "The First Direct Measurements of Surface Magnetic Fields on Very Low Mass Stars". The Astrophysical Journal. 656 (2): 1121–1135. doi:10.1086/510304.
- ^ Poveda, Arcadio; Allen, Christine; Herrera, Miguel Angel (1996). "Chromospheric Activity, Stellar Winds and Red Stragglers". Workshop on Colliding Winds in Binary Stars to Honor Jorge Sahade. 5. Universidad Nacional Autonoma de Mexico. hlm. 16–20.
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