Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-28T06:57:40.854Z Has data issue: false hasContentIssue false
  • English
  • Français

Multi-wavelength Observations of Novae in Outburst

Published online by Cambridge University Press:  12 April 2016

S. Starrfield
S. Starrfield*
Affiliation:
IGPP and Theoretical Division, Los Alamos National Laboratory and Department of Physics and Astronomy, Arizona State University

Extract

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.

A nova outburst is the second most violent explosion that can occur in a galaxy. While less violent than a supernova explosion, novae are considerably more frequent. More than 250 have been observed in the last century and there were more than a dozen novae being observed in outburst when this review was written. Over the past few years they have been studied at wavelengths ranging from the radio to the X-ray and these data have provided exciting new information about the nova outburst. For example, IUE studies have shown that there are two classes of novae; those that occur on carbon-oxygen white dwarfs and those that occur on oxygen-neon-magnesium white dwarfs. EXOSAT observations have shown that an intense X-ray emitting source exists in the system for years after the initial outburst has been discovered and radio studies have found that some novae are ejecting material in jets. IR studies have found high excitation coronal lines, dust formation, and have provided accurate distances. Optical studies have provided determinations of densities and temperatures in the ejecta and have discovered a class of novae that occur on strongly magnetized white dwarfs. There have been predictions but no detections of γ-ray emission. Finally, novae are time dependant and simultaneous or contemporaneous observations are required in order to learn as much as possible about the characteristics of the outburst.

Type
1b. Novae During Outbursts
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 127 - 137
Copyright
Copyright © Springer-Verlag 1990

References

Abbott, D.C. 1982, Ap. J., 259, 282.Google Scholar
Boyarchuk, A.A., Galkina, T.S., Krasnobabtsev, V.I., Rachkovskaya, T.M., and Sha-khovskaya, N.I. 1977, Sov. A. J., 21, 257.Google Scholar
Castor, J.I., Abbott, D.C., and Klein, R.I. 1975, Ap. J., 195, 157.Google Scholar
Cohen, J.G. 1985, Ap. J., 292, 90.Google Scholar
Ferland, G.J. and Shields, G.A. 1978a, Ap. J., 226, 172.Google Scholar
Ferland, G.J., and Shields, G.A. 1978b, Ap. J. (Letters), 224, L15.Google Scholar
Gallagher, J.S., and Ney, E.P. 1976, Ap. J. (Letters), 204, L35.Google Scholar
Gallagher, J.S. and Starrfield, S.G. 1976, M.N.R.A.S., 176, 53.Google Scholar
Gallagher, J.S. and Starrfield, S.G. 1978, Ann. Rev. Astr. and Ap., 16, 171.Google Scholar
Gehrz, R.D. 1988, Ann. Rev. Astr. and Ap., 26, 377.CrossRefGoogle Scholar
Gehrz, R.D., Grasdalen, G.L., Greenhouse, M., Hackwell, J.A., Hayward, T., and Bentley, A.F. 1986, Ap. J. (Letters), 308, L63.Google Scholar
Krautter, J., and Williams, R.E. 1989, Astrophys. J., 341, p. 968.Google Scholar
Lance, C.M., McCall, M.M., and Uomoto, A.K. 1988, Ap. J. Supp., 66, 151.Google Scholar
MacDonald, J. 1980, M.N.R.A.S., 191, 933.CrossRefGoogle Scholar
MacDonald, J., Fujimoto, M.Y., and Truran, J.W. 1985, Ap. J., 294, 263.Google Scholar
Mason, K.O., Córdova, F.A., Bode, M.F., and Barr, P. 1986, in RS Oph and the Recurrent Nova Phenomenon, ed. Bode, M.F. (VNU Press; Utrecht), p 167.Google Scholar
McLaughlin, D.B. 1960, in Stellar Atmospheres: Stars and Stellar Systems VI, ed. Greenstein, J.S. (Chicago: University of Chicago Press), p. 585.Google Scholar
Ögelman, H., Krautter, J., and Beuermann, K. 1987, Astr. Ap., 177, 110.Google Scholar
Paczynski, B. 1971, Acta Astron., 21, 271.Google Scholar
Shara, M.M. 1989, Public. Astron. Soc. pac., 101, p. 5.Google Scholar
Snijders, M.A.J., Batt, T.J., Roche, P.F., Seaton, M.J., Morton, D.C., Spoelstra, T.A.T., and Blades, J.C. 1987, M.N.R.A.S., 228, 329.Google Scholar
Sparks, W.M., Starrfield, S., Truran, J.W., and Kutter, G.S. 1988, in Atmospheric Phenomena in Stellar Explosions, ed. Nomoto, K., (Springer-Verlag: Heidelberg), p. 234.Google Scholar
Starrfield, S. 1979, in White Dwarfs and Variable Degenerate Stars, ed. Van Horn, H.M. and Weidemann, V. (Rochester: University of Rochester), p. 274.Google Scholar
Starrfield, S. 1986, in Radiation Hydrodynamics, ed. Mihalas, D., and Winkler, K.-H., (Dordrecht: Reidel), p. 225.Google Scholar
Starrfield, S. 1988, in Multiwavelength Astrophysics, ed. Cordova, F.A., (Cambridge:University Press), p. 159.Google Scholar
Starrfield, S. 1989, in The Classical Nova, ed. Evans, N., and Bode, M., (New York:Wiley), p. 39.Google Scholar
Starrfield, S., Sparks, W.M., and Truran, J.W. 1985 Ap. J., 291, 136.CrossRefGoogle Scholar
Starrfield, S., Sparks, W.M., and Truran, J.W. 1986, Ap. J. (Letters), 303, L5.Google Scholar
Starrfield, S., Sparks, W.M. and Truran, J.W. 1974, Ap. J. Suppl, 28, 247.CrossRefGoogle Scholar
Starrfield, S., Truran, J.W. and Sparks, W.M. 1978, Ap. J., 226, 186.Google Scholar
Starrfield, S., Truran, J.W., Sparks, W.M., and Krautter, J. 1989, in The Future of EUV Astronomy, ed. Malina, R., in press.Google Scholar
Starrfield, S., Truran, J.W., Sparks, W.M. and Kutter, G.S. 1972, Ap. J., 176, 169.Google Scholar
Stryker, L.L., Hestand, J., Starrfield, S., Wehrse, R., and Shaviv, G. 1988, in A Decade of UV Astronomy with the IUE Satellite, ed. Rolfe, E., (Noordwijk:Estec Publications: SP- 263), p. 149.Google Scholar
Truran, J.W. 1982, in Essays in Nuclear Astrophysics, ed. Barnes, C.A., Clayton, D.D., and Schramm, D. (Cambridge: Cambridge U. Press), p. 467.Google Scholar
Truran, J.W., and Livio, M. 1986, Ap. J., 308, 721.CrossRefGoogle Scholar
Williams, R.E., Sparks, W.M., Gallagher, J.S., Ney, E.P., Starrfield, S., and Truran, J.W. 1981, Ap. J., 251, 221.CrossRefGoogle Scholar
Williams, R.E., Sparks, W.M., Ney, E.P., Starrfield, S., and Truran, J.W. 1985, Mon. Not. Roy. Astron. Soc, 212, 753.Google Scholar