Hostname: page-component-cc8bf7c57-8cnds Total loading time: 0 Render date: 2024-12-12T07:40:19.879Z Has data issue: false hasContentIssue false

Are Novae Standard Candles?

Published online by Cambridge University Press:  12 April 2016

Shlomi Pistinner
Affiliation:
Department of Physics, Ben-Gurion University, Beer Sheba 84105, Israel
Giora Shaviv
Affiliation:
Department of Physics, Technion, Haifa 32000, Israel
Peter H. Hauschildt
Affiliation:
Department of Physics & Astronomy, Arizona State University, Tempe, AZ 85287-1504, USA
Sumner Starrfield
Affiliation:
Department of Physics & Astronomy, Arizona State University, Tempe, AZ 85287-1504, USA

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.

Novae in outburst can be used as distance indicators. The distance measurement process is considerably simplified if novae could be regarded as standard candles. The term standard candles in the context of this paper means that the absolute magnitude at maximum for different novae is, to a good approximation, constant. The t3Mb diagram (Schmidet 1957) implies that this is the case for M31 and LMC novae (Della Valle & Livio 1995). However, this conclusion does not necessarily apply to non Local Group novae (Livio 1992; Della Valle & Livio 1995); for example the Virgo novae are not similar to Local Group novae (Della Valle & Livio 1995). Here we focus on a question of principle, namely: Does the fact that novae have similar spectra imply that they have similar luminosities?

Type
Novae & Symbiotic Stars
Copyright
Copyright © Kluwer 1996

References

Della Valle, M., Livio, M., 1995, Ap. J., 452, 704 CrossRefGoogle Scholar
Hauschildt, P.H., Wehrse, R., Starrfleld, S., Shaviv, G., 1992, Ap. J., 393, 307 CrossRefGoogle Scholar
Hauschildt, P.H., Starrfleld, S., Austin, S., et al., 1994, Ap. J., 422, 831 CrossRefGoogle Scholar
Hauschildt, P.H., Starrfleld, S., Shore, M., et al., 1995, Ap. J., 447, 829 CrossRefGoogle Scholar
Livio, M., 1992, Ap. J., 393, 516 CrossRefGoogle Scholar
Pistinner, S., Shaviv, G., Hauschildt, P.H., Starrfleld, S., 1995, Ap. J., 451, 724 CrossRefGoogle Scholar
Schmidet, Th., 1957, Z. Astrophys., 41, 182 Google Scholar
Schuster, A., 1905, Ap. J., 21, 1 CrossRefGoogle Scholar