XMM-Newton Proposal 02019101

Details XMM-Newton Proposal 02019101 XMM-Newton Proposal 02019101

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..104m&link_type=abstract

XMM-Newton Proposal ID #02019101

Physics

Vxr 80, Xmm-Newton Proposal 02019101

Scientific paper

We propose to observe two young fast rotating stars observed with ROSAT in the supersaturation regime. We aim at detecting rotational modulation in their X-ray emission as recently found for VXR45, a star with similar rotational properties observed by us with XMM/Newton. If rotational modulation is a general characteristic of supersaturated stars, we will be able to determine the presence of an asymmetric distribution of coronal structures in such stars and from their (or lack of) spectral variations, to infer the characteristics of such structures constraining the properties of the underlying dynamo.

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