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Observational studies of pre-main-sequence evolution

Cohen, M., Kuhi, L. V.·1979·The Astrophysical Journal Supplement Series

Abstract

Optical scanner data from 4270 to 6710 A with a resolution of 7 A were obtained for some 500 H-alpha stars. The data were used to obtain spectral types, reddening coefficients, and emission line strengths; in addition, they are combined with IR broadband measurements out to 3.5 microns to provide bolometric luminosities and effective temperatures. H-R diagrams are presented for the Taurus-Auriga complex, Orion, NGC 2264, NGC 7000/IC 5070, and the Rho Ophiuci association. Some general conclusions are presented.

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Metadata

Authors
Cohen, M., & Kuhi, L. V.
Venue
The Astrophysical Journal Supplement Series
Published
1979-12
Volume
41
Pages
743
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W2021272563
Cited by
800
References
0
Type
conference abstract
Language
en
Open access
closed

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CoChat. (2026). Citation check: Observational studies of pre-main-sequence evolution. https://app.cochat.ai/papers/10.1086/190641
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Cohen, M., & Kuhi, L. V. (1979). Observational studies of pre-main-sequence evolution. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/190641

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