Hostname: page-component-8448b6f56d-qsmjn Total loading time: 0 Render date: 2024-04-16T04:01:59.077Z Has data issue: false hasContentIssue false
  • English
  • Français

The AFCRL Catalogue: Some Southern Sources Studied

Published online by Cambridge University Press:  25 April 2016

A. J. Longmore ,
A. R. Hyland  and
D. A. Allen
A. J. Longmore
Affiliation:
U.K. Schmidt Telescope Unit, Coonabarabran
A. R. Hyland
Affiliation:
Mount Stromio and Siding Spring Observatory, The Australian National University
D. A. Allen
Affiliation:
U.K. Schmidt Telescope Unit, Coonabarabran
Get access Rights & Permissions [Opens in a new window]

Extract

The strategic value of infrared sensing has prompted military development — mostly in the USA — of detectors for 8-30 μm far more sensitive than any commercially available. In 1970-72 the Air Force Cambridge Research Laboratories conducted a rocket-borne survey of the sky N. of about -35° dec at 4,11 and 20 μm. Although this survey was initially classified, a small number of preliminary versions of it were distributed to selected infrared astronomers based at U.S. institutions.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 47 - 49
Copyright
Copyright © Astronomical Society of Australia 1976

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Allen, D. A., Harvey, P. M. and Swings, J. P., Astron. and Astrophys., 20, 333 (1972).Google Scholar
Allen, D. A., Hyland, A. R. and Longmore, A. J., Mon. Not. R. Astron. Soc, 175, p. 61 (1976).Google Scholar
Beckwith, S., Evans, N. J., Becklin, E. E. and Neugebauer, G., ‘Infrared Observations of the Mon R2 Association’, Astrophys. J., (in press) (1976).Google Scholar
Cohen, M., Astrophys. J., 185, L75 (1973).CrossRefGoogle Scholar
Cohen, M., Astron. J., 80, 125 (1975); includes identifications by Merrill, .CrossRefGoogle Scholar
Cohen, M., Astrophys, J., 203, 169 (1976).CrossRefGoogle Scholar
Cohen, M. et al, Astrophys. J., 196, 179 (1975), (16 authors).CrossRefGoogle Scholar
Cohen, M., Barlow, M. J. and Kuhi, L. V., Astron. and Astrophys., 40, 291 (1975).Google Scholar
Cohen, M. and Kuhi, L. V., ‘Spectroscopic Observations of Optically Identified AFCRL Infrared Sources’, Pubi. Astron. Soc. Pacific, (in press) (1976).CrossRefGoogle Scholar
Hansen, O. L. and Blanco, V. M., Astron. J., 78, 669 (1973).CrossRefGoogle Scholar
Hansen, O. L. and Blanco, V. U., Astron. J., 80, 1011 (1975).CrossRefGoogle Scholar
Hoffmann, W. F., Frederick, C. L. and Emery, R. S., Astrophys. J., 170, L89 (1971).CrossRefGoogle Scholar
Hyland, A. R., Becklin, E. E., Frogel, J. A. and Neugebauer, G., Astron. and Astrophys., 16, 204 (19.72).Google Scholar
Keenan, P. C., Astrophys. J., 120, 484 (1954).CrossRefGoogle Scholar
Keenan, P. C., Chapter 8 of ‘Basic Astronomical Data’ ed. K.Aa. Strand, University of Chicago Press (1963).Google Scholar
Lebofsky, M. J., Kleinmann, S. G. and Rieke, G. H., Bull. Amer. Astron. Soc, 7, 410 (1975).Google Scholar
Low, F. J., AFCRL Technical Report 73–0371 (1973).Google Scholar
Neugebauer, G. and Leighton, R. B., NASA SP-3047 (1969).Google Scholar
Ney, E. P., Merrill, K. M., Becklin, E. E., Neugebauer, G. and Wynn Williams, C. G., Astrophys. J., 198, L129 (1975).CrossRefGoogle Scholar
Rybski, P.M., I.A.U. Symposium, 50, 96 (1973).Google Scholar
Stromgren, B. and Gyldenkerne, Y., Astrophys. J., 121, 43 (1955).CrossRefGoogle Scholar
Vogt, S. S., Astron. J., 78, 389 (1973).CrossRefGoogle Scholar
Walker, R. G. and Price, S. D., AFCRL Technical Report 75-0373 (1975).Google Scholar
Westbrook, W. E., Becklin, E. E., Merrill, K. M., Neugebauer, G., Schmidt, M., Willner, S. P., and Wynn-Williams, C. G., Astrophys. J., 202, 407(1975).CrossRefGoogle Scholar