Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-12-05T02:14:20.236Z Has data issue: false hasContentIssue false

Probe of the Nearby Interstellar Medium by the Vacant Line of Sight to β CMa

Published online by Cambridge University Press:  12 April 2016

C. Gry
Affiliation:
ESA Satellite Tracking Station, Madrid
D.G. York
Affiliation:
University of Chicago, U.S.A.
A. Vidal-Madjar
Affiliation:
Institut d'Astrophysique, Paris

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.

The line of sight to βCMa has been probed by Copernicus observations. This particular line of sight is remarkable for the low mean densities. We find n̄H ∼ .002 cm-3. However we can distinguish two separate regions:

1) A local nearby HI region extends over a few parsecs from the sun with a density of the order of 0.1 cm-3 and a temperature of 11000 to 12500 K.

2) An HII region lies somewhere beyond the HI region and is spread over about 60pc. Its total hydrogen mean density is of the same order as the HI region, i.e. of ∼0.1 cm-3 and it contains only elements in low ionization state. All the data are coherent with the picture of a cloud in ionization equilibrium at T ∼ 23 000° K.

Type
Ultraviolet and EUV Absorption Studies
Copyright
Copyright © NASA 1984

References

Bruhweiler, F.C.,Kondo, Y.,1982, Ap.J. 259, 232 Google Scholar
Ferlet, R., 1981, A.and A.,,98, LlGoogle Scholar
Spitzer, L., Jenkins, E.B., 1975, Ann.Rev.Astron.Astrophys.13, 133 Google Scholar
Vidal-Madjar, A., Laurent, C., Bonnet, R.M., York, D.G., 1977, Ap.J.,211, 91 CrossRefGoogle Scholar
York, D.G., 1983, Ap.J.,264, 172 Google Scholar
York, D.G.,Kinahan, B.F., 1979,Ap.J.,264, 172 Google Scholar
York, D.G., Spitzer, L., Bohlin, R.C., Hill, J., Jenkins, E.B., Savage, B.D.,Snow, T.P., 1983, Ap.J., 266, L55Google Scholar