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IRAS 19475+3119 is a protoplanetary nebula in the constellation of Cygnus, 15,000 light-years away. The central star, V2513 Cygni, is an F-type post-AGB star.

IRAS 19475+3119

IRAS 19474+3119
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 49m 29.5618s[1]
Declination +31° 27′ 16.249″[1]
Apparent magnitude (V) 9.33 - 9.50[2]
Characteristics
Evolutionary stage Protoplanetary nebula
Spectral type F3 Ibe[3]
Variable type SRd[2]
Astrometry
Proper motion (μ) RA: −0.156[1] mas/yr
Dec.: −1.684[1] mas/yr
Parallax (π)0.3159 ± 0.0209 mas[1]
Distance4,900[4] pc
Details
Mass0.63[4] M☉
Radius58[4] R☉
Luminosity8,300[4] L☉
Surface gravity (log g)0.5[4] cgs
Temperature7,200[3] K
Metallicity [Fe/H]−0.25[3] dex
Other designations
V2513 Cyg, BD+31°3797, HD 331319
Database references
SIMBADdata

The brightest portion of the nebula shows a quadrupolar structure, with elongated bipolar lobes, all surrounded by a faint halo.[5]

A visual band light curve for V2513 Cygni, adapted from Hrivnak et al. (2018)[6]
A visual band light curve for V2513 Cygni, adapted from Hrivnak et al. (2018)[6]

The distance is essentially unknown. Assumptions about the luminosity have been used to estimate the distance and other stellar parameters. At an assumed kinematical distance of 4.9 kpc, the luminosity is 8,300 L☉ and the radius 58 R☉.[4] The star was originally at least 2.5 M☉ and is now 0.63 M☉.[5] Assuming a luminosity of 3,500 L☉, the distance becomes 1.5 kpc.[7] Estimates based on the oxygen spectral line strengths give much higher values luminosities with an absolute magnitude of at least −8.[3]

The central star is variable, from about magnitude 9.33 to 9.50. A primary period of 41 days has been determined, but a slightly shorter secondary period leads to long beats causing variations in the amplitude and apparent period from year to year. The variations are caused by stellar pulsations, with the star being brightest when it is hottest. The temperature varies by up to 400 K.[8]


References


  1. 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.
  2. Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  3. Klochkova, V. G.; Panchuk, V. E.; Tavolzhanskaya, N. S. (2002). "HD 331319: A Post-AGB F Supergiant with He I Lines". Astronomy Letters. 28 (1): 49–62. Bibcode:2002AstL...28...49K. doi:10.1134/1.1434453. S2CID 120988304.
  4. Hsu, Ming-Chien; Lee, Chin-Fei (2011). "An Envelope Disrupted by a Quadrupolar Outflow in the Pre-planetary Nebula IRAS 19475+3119". The Astrophysical Journal. 736 (1): 30. arXiv:1105.2410. Bibcode:2011ApJ...736...30H. doi:10.1088/0004-637X/736/1/30. S2CID 119192160.
  5. Sahai, Raghvendra; Sánchez Contreras, Carmen; Morris, Mark; Claussen, Mark (2007). "A Quadrupolar Preplanetary Nebula: IRAS 19475+3119". The Astrophysical Journal. 658 (1): 410–422. Bibcode:2007ApJ...658..410S. doi:10.1086/511294.
  6. Hrivnak, Bruce J.; Van de Steene, Griet; Van Winckel, Hans; Lu, Wenxian; Sperauskas, Julius (December 2018). "Variability in Proto-planetary Nebulae. V. Velocity and Light Curve Analysis of IRAS 17436+5003, 18095+2704, and 19475+3119". The Astronomical Journal. 156 (6). doi:10.3847/1538-3881/aaee69. Retrieved 31 December 2021.
  7. Vickers, Shane B.; Frew, David J.; Parker, Quentin A.; Bojičić, Ivan S. (2015). "New light on Galactic post-asymptotic giant branch stars - I. First distance catalogue". Monthly Notices of the Royal Astronomical Society. 447 (2): 1673. arXiv:1403.7230. Bibcode:2015MNRAS.447.1673V. doi:10.1093/mnras/stu2383. S2CID 119245776.
  8. Hrivnak, Bruce J.; Lu, Wenxian; Nault, Kristie A. (2015). "Variability in Proto-planetary Nebulae. IV. Light Curve Analysis of Four Oxygen-rich, F Spectral Type Objects". The Astronomical Journal. 149 (6): 184. arXiv:1503.09120. Bibcode:2015AJ....149..184H. doi:10.1088/0004-6256/149/6/184. S2CID 119266827.

На других языках

[de] IRAS 19475+3119

IRAS 19475+3119 ist ein Pre-Planetarischer Nebel im Sternbild Schwan, etwa 15.000 Lichtjahre entfernt. Eine Beobachtung bei 0,43 und 0,6 μm mit dem Hubble-Weltraumteleskop zeigt eine quadrupolare Struktur.[3]
- [en] IRAS 19475+3119


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