Pith. sign in

REVIEW

Emission Measure Distribution and Abundances Measurements During High-T Flares

Not yet reviewed by Pith; the record is open.

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/0511159 v1 pith:FZW2GHG5 submitted 2005-11-06 astro-ph

classification astro-ph
keywords duringflaredistributionemissionlargemeasuresigmaabundances
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The RSCVn system Sigma Geminorum was observed by XMM-Newton on April 2001 during a large flare. We model the emission measure distribution (EMD) during the flare and during a quiescence period. In the flare, a two phase behaviour is found in which the cool plasma (kT < 2 keV) is not disturbed while a large hot component, at temperatues of kT > 3 keV emerges. Fundamental limitations on EMD modeling of high temperature plasmas are then discussed, in the context of the Sigma Gem flare.

Discussion (0). Sign in to comment.

Pith tools