Pith. sign in

REVIEW

Gamma-ray emission of classical novae and its detectability by INTEGRAL

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/9812100 v1 pith:PDBU6WYR submitted 1998-12-04 astro-ph

M. Hernanz , J. Gomez-Gomar , J. Jose , A. Coc , J. Isern This is my paper · ORCID
classification astro-ph
keywords integralclassicaldetectabilitydifferentemissiongamma-raynovaepossible
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

A lot of information concerning the mechanism of nova explosions will be extracted from the possible future observations with INTEGRAL. In order to be prepared for this task, we are performing detailed models of the gamma-ray emission of classical novae, for a wide range of possible initial conditions. Spectra at different epochs after the explosion and light curves for the different lines (511, 478 and 1275 keV) and the continuum are presented, as well as the detectability distances with INTEGRAL spectrometer SPI. New results related to 18F synthesis related to very recent data of nuclear physics are advanced as preliminary.

Discussion (0). Continue with ORCID to comment.

Pith tools