Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-27T00:38:07.222Z Has data issue: false hasContentIssue false
  • English
  • Français

A Near–IR Survey of the Southern Galactic Plane

Published online by Cambridge University Press:  12 April 2016

D. Jack MacConnell ,
Robert F. Wing  and
H. Edgardo Costa
D. Jack MacConnell
Affiliation:
Astronomy Programs, Computer Sciences Corporation, Space Telescope Science Institute
Robert F. Wing
Affiliation:
Ohio State University
H. Edgardo Costa
Affiliation:
Universidad de Chile

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We describe a long term project to find faint, heavily-reddened, cool supergiants and carbon stars and to classify IRAS Point Sources within 6° of the southern galactic plane. Many new supergiants and carbon stars have been found, and thousands of IRAS Point Sources have had their spectral types determined.

Type
IX. Galactic Structure and Stellar Surveys
Information
International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 316 - 319
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Blanco, V.M. & Münch, L., 1955, Bol. Ton. Tac., No. 12, 17 Google Scholar
MacConnell, D.J., Wing, R.F. & Costa, E., 1992, AJ, 104, 821 CrossRefGoogle Scholar
Meylan, G. & Maeder, A., 1983, A&A, 124, 84 Google Scholar
Nassau, J.J., Blanco, V.M. & Morgan, W.W., 1954, ApJ, 120, 478 CrossRefGoogle Scholar
Wing, R.F., 1971, In Proceedings of the Conference on Late-Type Stars, Lockwood, G.W. & Dyck, H.M., eds, KPNO Contrib. No. 554, 145 Google Scholar