The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities

2); (2) INAF/IASF Milano (3) INAF/IASF Palermo; A. Paizis (2); Como; Italy); L. Ducci (1; L. Sidoli (2); P. Romano (3); S. Mereghetti (2) ((1) Universit\`a degli Studi dell'Insubria

REVIEW

The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities

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 1003.5829 v1 pith:Z6CYBPE2 submitted 2010-03-30 astro-ph.HE

The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities

L. Ducci (1 , 2) , L. Sidoli (2) , P. Romano (3) , A. Paizis (2) , S. Mereghetti (2) ((1) Universit\`a degli Studi dell'Insubria , Como , (2) INAF/IASF Milano (3) INAF/IASF Palermo

show 1 more author

Italy)

This is my paper

classification astro-ph.HE

keywords x-raybinarieshighmassmodelwindbehaviourclasses

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

We have developed a clumpy stellar wind model for OB supergiants in order to compare predictions of this model with the X-ray behaviour of both classes of persistent and transient High Mass X-ray Binaries (HMXBs).

The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities

discussion (0)