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Photometry of the FU Orionis stars V1057 cygni and V1515 Cygni

Journal Article · · Publ. Astron. Soc. Pac.; (United States)
DOI:https://doi.org/10.1086/130213· OSTI ID:5110877
UBVR photoelectric data were obtained for V1057 Cyg in 1975, 1976, and 1977. Its rate of fading has slowed to 0./sup m/0005 per day. Another FU Ori type object, V1515 Cyg, is found to have photoelectric colors essentially the same as V1057 Cyg.
OSTI ID:
5110877
Journal Information:
Publ. Astron. Soc. Pac.; (United States), Journal Name: Publ. Astron. Soc. Pac.; (United States) Vol. 89:531; ISSN PASPA
Country of Publication:
United States
Language:
English

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