Pith. sign in

REVIEW

Photometric and spectroscopic variations of the Be star HD 112999

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 1305.7098 v1 pith:BTKU5NON submitted 2013-05-30 astro-ph.SR

M. A. Corti , R. C. Gamen , Y. J. Aidelman , G. A. Ferrero , W. A. Weidmann This is my paper
classification astro-ph.SR
keywords spectroscopicstarslinesphotometricstartransienttypeanalysis
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Be objects are stars of B spectral type showing lines of the Balmer series in emission. The presence of these lines is attributed to the existence of an extended envelope, disk type, around them. Some stars are observed in both the Be and normal B-type spectroscopic states and they are known as transient Be stars. In this paper we show the analysis carried out on a new possible transient Be star, labelled HD 112999, using spectroscopic optical observations and photometric data.

Discussion (0). Sign in to comment.

Pith tools