Gamma rays and X-rays from classical novae

James W. Truran, Sumner Starrfield

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Citations (Scopus)

Abstract

The thermonuclear runaways occurring in accreted hydrogen shells on white dwarfs in close binary systems, that define the outbursts of the classical novae, provide an environment in which explosive hydrogen burning can produce significant concentrations of the interesting longer lived radioactive isotopes 7 Be (τ 1/2 =53.28 days), 22 Na,( τ 1/2 =2.605 years), and 26 Al (τ 1/2 =7.2×10 5 years), as well as of the short-lived positron-unstable isotopes 13 N, 14 O, 15 O, 17 F, and 18 F. It follows that nearby novae may produce flux levels of gamma rays, during several phases of their evolution, that are detectible with the Compton Gamma Ray Observatory. We briefly review the theoretical and observational picture with regard to the identified potential sources of gamma rays from novae. In particular, we reexamine the current situation regarding the production of 7 Be, 22 Na, and 26 Al in nova outbursts, and provide updated estimates of the expected fluxes of 7 Be and 22 Na gamma rays from individual nova events. Expectations for X-rays from novae are also noted.

Original languageEnglish (US)
Title of host publicationCompton Gamma-Ray Observatory
EditorsNeil Gehrels, Michael W. Friedlander, Daryl J. Macomb
PublisherAmerican Institute of Physics Inc.
Pages163-167
Number of pages5
ISBN (Electronic)1563961040
DOIs
StatePublished - Jan 1 1993
EventCompton Symposium - St. Louis, United States
Duration: Oct 15 1992Oct 17 1992

Publication series

NameAIP Conference Proceedings
Volume280
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceCompton Symposium
CountryUnited States
CitySt. Louis
Period10/15/9210/17/92

Fingerprint

novae
gamma rays
x rays
Gamma Ray Observatory
hydrogen
radioactive isotopes
positrons
isotopes
estimates

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Truran, J. W., & Starrfield, S. (1993). Gamma rays and X-rays from classical novae. In N. Gehrels, M. W. Friedlander, & D. J. Macomb (Eds.), Compton Gamma-Ray Observatory (pp. 163-167). (AIP Conference Proceedings; Vol. 280). American Institute of Physics Inc.. https://doi.org/10.1063/1.44165

Gamma rays and X-rays from classical novae. / Truran, James W.; Starrfield, Sumner.

Compton Gamma-Ray Observatory. ed. / Neil Gehrels; Michael W. Friedlander; Daryl J. Macomb. American Institute of Physics Inc., 1993. p. 163-167 (AIP Conference Proceedings; Vol. 280).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Truran, JW & Starrfield, S 1993, Gamma rays and X-rays from classical novae. in N Gehrels, MW Friedlander & DJ Macomb (eds), Compton Gamma-Ray Observatory. AIP Conference Proceedings, vol. 280, American Institute of Physics Inc., pp. 163-167, Compton Symposium, St. Louis, United States, 10/15/92. https://doi.org/10.1063/1.44165
Truran JW, Starrfield S. Gamma rays and X-rays from classical novae. In Gehrels N, Friedlander MW, Macomb DJ, editors, Compton Gamma-Ray Observatory. American Institute of Physics Inc. 1993. p. 163-167. (AIP Conference Proceedings). https://doi.org/10.1063/1.44165
Truran, James W. ; Starrfield, Sumner. / Gamma rays and X-rays from classical novae. Compton Gamma-Ray Observatory. editor / Neil Gehrels ; Michael W. Friedlander ; Daryl J. Macomb. American Institute of Physics Inc., 1993. pp. 163-167 (AIP Conference Proceedings).
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