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Alpha Pyxidis

Alpha Pyxidis (afgekort as α Pyx) is ’n reusester in die sterrebeeld Kompas (Pyxis) en die helderste ster in die sterrebeeld. Dit is ’n Beta Cephei-veranderlike en het ’n sterreklassifikasie van B1,5 III. Sy massa is meer as 10 keer dié van die Son en sy radius ses keer die Son s’n. Sy oppervlaktemperatuur is 24 300 K en sy ligsterkte is sowat 10 000 keer dié van die Son.[1][5][7]

Alpha Pyxidis
Alpha Pyxidis se ligging (in die rooi sirkel).
Alpha Pyxidis se ligging (in die rooi sirkel).
Sterrebeeld Kompas
Spektraaltipe B1.5 III[1]
Soort Reusester
Waarnemingsdata (Epog J2000)
Regte klimming 08h 43m 35.53756s[2]
Deklinasie -33° 11′ 10.9898″[2]
Skynmagnitude (m) 3,67[3]
Absolute magnitude (M) -3,47[4]
B-V-kleurindeks  -0,19[3]
U-B-kleurindeks  -0,84[3]
Besonderhede
Massa (M☉) 10,7[5]
Radius (R☉) 6,3 ± 1,0[6]
Ligsterkte (L☉) 10 000[5]
Temperatuur (K) 24 300[7]
Rotasiespoed (km/s) 11[8]
Metaalinhoud [Fe/H] -0,18[7]
Eienskappe
Veranderlikheid Beta Cephei[5]
Ander name
CPD−32° 2399, FK5 327, HD 74575, HIP 42828, HR 3468, SAO 199546.[9]
Portaal  Portaalicoon   Sterrekunde

Verwysings

wysig
  1. ↑ 1,0 1,1 Hiltner, W. A.; Garrison, R. F.; Schild, R. E. (Julie 1969). "MK Spectral Types for Bright Southern OB Stars". Astrophysical Journal. 157: 313. Bibcode:1969ApJ...157..313H. doi:10.1086/150069.
  2. ↑ 2,0 2,1 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V 
  3. ↑ 3,0 3,1 3,2 Fernie, J. D. (Mei 1983). "New UBVRI photometry for 900 supergiants". Astrophysical Journal Supplement Series. 52: 7–22. Bibcode:1983ApJS...52....7F. doi:10.1086/190856.
  4. ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A. 
  5. ↑ 5,0 5,1 5,2 5,3 Hubrig, S.; et al. (Januarie 2009). "New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars". Astronomische Nachrichten. 330 (4): 317. arXiv:0902.1314. Bibcode:2009AN....330..317H. doi:10.1002/asna.200811187.
  6. ↑ Hubrig, S.; Ilyin, I.; Schöller, M.; Briquet, M.; Morel, T.; De Cat, P. (Januarie 2011), "First Magnetic Field Models for Recently Discovered Magnetic β Cephei and Slowly Pulsating B Stars", The Astrophysical Journal Letters 726 (1): L5, doi:10.1088/2041-8205/726/1/L5, Bibcode: 2011ApJ...726L...5H, http://orbi.ulg.ac.be/bitstream/2268/81132/1/apjl_726_1_5.pdf 
  7. ↑ 7,0 7,1 7,2 Kilian, J. (Februarie 1994). "Chemical abundances in early B-type stars. 5: Metal abundances and LTE/NLTE comparison". Astronomy and Astrophysics. 282 (3): 867–873. Bibcode:1994A&A...282..867K.
  8. ↑ Nieva, M. F.; Przybilla, N. (April 2008). "Carbon abundances of early B-type stars in the solar vicinity. Non-LTE line-formation for C II/III/IV and self-consistent atmospheric parameters". Astronomy and Astrophysics. 481 (1): 199–216. arXiv:0711.3783. Bibcode:2008A&A...481..199N. doi:10.1051/0004-6361:20078203.
  9. ↑ "NSV 4220 -- Variable Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Besoek op 23 Februarie 2010.

Eksterne skakels

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