P Cygni
Lokasi P Cygni (dilingkari merah)
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Data pengamatan Epos J2000 Ekuinoks J2000
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Rasi bintang
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Cygnus
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Asensio rekta
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20j 17m 47.2018d[1]
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Deklinasi
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+38° 01′ 58.549″[1]
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Magnitudo tampak (V)
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4.82[2] (3 to 6[3])
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Ciri-ciri
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Kelas spektrum
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B1Ia+[4]
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Indeks warna U−B
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-0.58[4]
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Indeks warna B−V
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+0.42[4]
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Jenis variabel
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LBV[3]
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Astrometri |
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Kecepatan radial (Rv) | -8.9[5] km/s |
Gerak diri (μ) | RA: -3.53[1] mdb/thn Dek.: -6.88[1] mdb/thn |
Paralaks (π) | 0,32±0,16[1] mdb |
Jarak | 1,700[6] pc |
Magnitudo mutlak (MV) | −7.9[7] |
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Detail |
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Massa | 30[8] M☉ |
Radius | 76[9] R☉ |
Luminositas | 610,000[9] L☉ |
Gravitasi permukaan (log g) | 1.2[6] |
Suhu | 18,700[9] K |
Metalisitas | 0.29[9] He/H |
Kecepatan rotasi (v sin i) | 35[6] km/s |
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Penamaan lain |
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Nova Cyg 1600, 34 Cyg, JP11 3218, TD1 26474, GSC 03151-03442, TYC 3151-3442-1, AG+37° 1953, 2MASS J20174719+3801585, ALS 11097, HD 193237, MCW 849, BD+37°3871, Hen 3-1871, PLX 4837, CEL 5017, PPM 84645, P Cyg, RAFGL 5493S, GC 28218, HIP 100044, ROT 2959, GCRV 12673, HR 7763, SAO 69773, AAVSO 2014+37A |
Referensi basis data |
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SIMBAD | data |
P Cygni (34 Cyg) adalah bintang variabel yang terletak di konstelasi Cygnus. Sebutan "P" pada awalnya dinyatakan oleh Johann Bayer di Uranometria untuk nova. Berjarak sekitar 5.000 hingga 6.000 tahun cahaya (1.500–1.800 parsec) dari Bumi, P Cygni adalah bintang hiper raksasa variabel biru bercahaya (VBR) tipe spektral B1Ia+ yang merupakan salah satu bintang paling bercahaya di Bima Sakti.
- ^ a b c d e Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752 . Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ^ Ducati, J. R. (2002). "VizieR On-line Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237: 0. Bibcode:2002yCat.2237....0D.
- ^ a b Samus, N. N.; Durlevich, O. V.; et al. (2004). "VizieR Online Data Catalog: Combined General Catalogue of Variable Stars (Samus+ 2004)". VizieR On-line Data Catalog: II/250. Originally Published in: 2004yCat.2250....0S. 2250: 0. Bibcode:2004yCat.2250....0S.
- ^ a b c Smith, L. J.; Crowther, P. A.; Prinja, R. K. (1994). "A study of the luminous blue variable candidate He 3-519 and its surrounding nebula". Astronomy and Astrophysics. 281: 833. Bibcode:1994A&A...281..833S.
- ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053 . Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.
- ^ a b c Najarro, F.; Hillier, D. J.; Stahl, O. (1997). "A spectroscopic investigation of P Cygni. I. H and HeI lines". Astronomy and Astrophysics. 326: 1117. Bibcode:1997A&A...326.1117N.
- ^ Van Genderen, A. M. (2001). "S Doradus variables in the Galaxy and the Magellanic Clouds". Astronomy and Astrophysics. 366 (2): 508–531. Bibcode:2001A&A...366..508V. doi:10.1051/0004-6361:20000022 .
- ^ Balan, Aurelian; Tycner, C.; Zavala, R. T.; Benson, J. A.; Hutter, D. J.; Templeton, M. (2010). "THE SPATIALLY RESOLVED Hα-EMITTING WIND STRUCTURE OF P CYGNI". The Astronomical Journal. 139 (6): 2269. arXiv:1004.0376 . Bibcode:2010AJ....139.2269B. doi:10.1088/0004-6256/139/6/2269.
- ^ a b c d Najarro, F. (2001). "Spectroscopy of P Cygni". P Cygni 2000: 400 Years of Progress. 233: 133. Bibcode:2001ASPC..233..133N.