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Observational studies of pre-main-sequence evolution
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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Cited by
A [ITAL]Hipparcos[/ITAL] Census of the Nearby OB Associations
de Zeeuw, P. T., Hoogerwerf, R., de Bruijne, J. H. J., Brown, A. G. A., & Blaauw, A. (1999) · The Astronomical Journal · doi:10.1086/300682 · Cited by 1,317
Protoplanetary disk structures in Ophiuchus
Andrews, S. M., Wilner, D. J., Hughes, A. M., Qi, C., & Dullemond, C. P. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/700/2/1502 · Cited by 709
Exploring the Full Stellar Population of the Upper Scorpius OB Association
Preibisch, T., Brown, A. G. A., Bridges, T., Guenther, E., & Zinnecker, H. (2002) · The Astronomical Journal · doi:10.1086/341174 · Cited by 349
Mannings, V., & Sargent, A. I. (1997) · The Astrophysical Journal · doi:10.1086/304897 · Cited by 332
An Assessment of Dynamical Mass Constraints on Pre–Main‐Sequence Evolutionary Tracks
Hillenbrand, L. A., & White, R. J. (2004) · The Astrophysical Journal · doi:10.1086/382021 · Cited by 319
Metadata
- Authors
- Cohen, M., & Kuhi, L. V.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- 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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