NGC 2264 and NGC 7000/IC revisited: A new search for emission H. cap alpha. stars
Journal Article
·
· Astron. J.; (United States)
OSTI ID:5662210
A slitless spectrographic search for H..cap alpha.. emission stars in NGC 2264 and NGC 7000/IC 5070 has revealed 18 new examples, most of which are presumably T Tau stars. An examination of all known T Tau stars in these fields has uncovered no events of the FU Ori type, except for that of V1057 Cyg. The incompleteness of the search as a function of magnitude and H..cap alpha.. strength is estimated by comparison with Herbig's survey (1954, 1958). It is found that for B<16.0, about 80% of the potential H..cap alpha.. emitters will be found in a survey with this equipment. These results, combined with an estimate of the volume occupied by the association in NGC 2264, yield a volume density of stars that show H..cap alpha.. emission (either now, or eventually if the area is surveyed repeatedly) brighter than B=19 of about 1.6 pc/sup -3/.
- Research Organization:
- Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz, California 95064
- OSTI ID:
- 5662210
- Journal Information:
- Astron. J.; (United States), Journal Name: Astron. J.; (United States) Vol. 85:3; ISSN ANJOA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BALMER LINES
EMISSION SPECTRA
ERUPTIVE VARIABLE STARS
LUMINOSITY
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
SPECTRA
SPECTROSCOPY
STARS
T TAURI STARS
VARIABLE STARS
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BALMER LINES
EMISSION SPECTRA
ERUPTIVE VARIABLE STARS
LUMINOSITY
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
SPECTRA
SPECTROSCOPY
STARS
T TAURI STARS
VARIABLE STARS