19 Vulpeculae

19 Vulpeculae
	19 Vulpeculae in the constellation Vulpecula.
Observation data; Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation	Vulpecula
Right ascension	20h 11m 47.97409s
Declination	26° 48′ 32.3663″
Apparent magnitude (V)	5.40
Distance	1,411 ly; (433 pc)
Spectral type	K2 IIIa
Other designations
	HD 192004, HR 7718, HIP 99518
Database references
SIMBAD	data

19 Vulpeculae (19 Vul) is an orange supergiant star (K3I), approximately 1,400 light years from Earth in the constellation Vulpecula and proximity of the open clusters NGC 6882 and NGC 6885 (Caldwell 37).

External links

19 Vulpeculae on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

References

^ ^a ^b ^c Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
^ Fernie, J. D. (1983). "New UBVRI photometry for 900 supergiants". Astrophysical Journal Supplement Series. 52: 7. Bibcode:1983ApJS...52....7F. doi:10.1086/190856.
^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.

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[hipparcos-1] Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.

[fernie-2] Fernie, J. D. (1983). "New UBVRI photometry for 900 supergiants". Astrophysical Journal Supplement Series. 52: 7. Bibcode:1983ApJS...52....7F. doi:10.1086/190856.

[perkins-3] Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.

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