Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-24T17:01:43.700Z Has data issue: false hasContentIssue false
  • English
  • Français

The Interaction of Nova Shells with the Interstellar Medium*

Published online by Cambridge University Press:  12 April 2016

H.W. Duerbeck
H.W. Duerbeck*
Affiliation:
Astronomisches Institut, Universität Münster, Münster, F.R.G.

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.

Decelerations of the shells around the novae V603 Aql, V476 Cyg, DQ Her and GK Per were determined from photographs and recent CCD observations. The deceleration is larger for higher expansion velocities, the mean half-lifetime, after which the expansion velocity has dropped to half its initial value, is 75 years.

Type
V. Nova and Dwarf Nova Outbursts
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 461 - 466
Copyright
Copyright © Reidel 1987

Footnotes

*

Based on observations obtained at the European Southern Observatory, La Silla, Chile, and at the Centro Astronomico Hispano-Aleman Calar Alto, operated by the Max-Planck-Institut fur Astronomie, Heidelberg

References

Adams, W.S.: 1941, Publ. Astr. Soc. Pacific 54, 229.Google Scholar
Adams, W.S.: 1944, Publ. Astr. Soc. Pacific 56, 213.Google Scholar
Aitken, R.G.: 1919, Publ. Astr. Soc. Pacific, 31, 283.Google Scholar
Aitken, R.G.: 1920, Publ. Astr. Soc. Pacific 54, 231.Google Scholar
Aitken, R.G.: 1921, Publ. Astr. Soc. Pacific 33, 219.Google Scholar
Baade, W.: 1940, Publ. Astr. Soc. Pacific 54, 229.Google Scholar
Baade, W.: 1942, Publ. Astr. Soc. Pacific, 54, 244.Google Scholar
Barnard, E.E.: 1918, Astrophys. J. 49, 199.Google Scholar
Barnard, E.E.: 1920, Publ. Astr. Soc. Pacific 32, 222.Google Scholar
Boyarchuk, A.A.: 1970, in IAU Symp. 39, “Interstellar Gas Dynamics”, H.J. Habing (ed.), p. 281.Google Scholar
Hubble, E.P., Duncan, J.C.: 1927, Astrophys. J. 66, 59.CrossRefGoogle Scholar
Kluyver, H.A.: 1951, in “Problems of Cosmic Aerodynamics”, Central Air Documents Office, Dayton p. 89.Google Scholar
Mustel, E.R., Boyarchuk, A.A.: 1970, Astrophys. Space Sci. 6, 183.CrossRefGoogle Scholar
Oort, J.H.: 1946, Mon. Not. R. astr. Soc. 106, 159.Google Scholar
Oort, J.H.: 1951, in “Problems of Cosmic Aerodynamics”, Central Air Documents Office, Dayton p. 118 Google Scholar
Seitter, W.C., Duerbeck, H.W.: 1986, in “RS Ophiuchi (1985) and the Recurrent Nova Phenomenon”, Bode, M.F. (ed.), VNU Press, Amsterdam (in press)Google Scholar
Williams, R.E., Woolf, N.J., Hege, E.K., Moore, R.C., Kopriva, D.A.: 1978, Astro phys. J. 224, 171.Google Scholar