Further Resolving the Puzzle of Hybrid Star X-rays

Details Further Resolving the Puzzle of Hybrid Star X-rays Further Resolving the Puzzle of Hybrid Star X-rays

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hst..prop10767a&link_type=abstract

HST Proposal ID #10767

Computer Science

Hst Proposal Id #10767

Scientific paper

Do Alpha TrA {K2II} and Beta Ind {K1II} have previously unrecognized X-ray active dwarf companions, leading us astray concerning the coronal properties of the "hybrid-chromosphere" class? Establishing the true X-ray luminosities of the hybrids is a basis for understanding magnetic field generation in evolved supergiants, the driving of their winds, and the seeding of coronal conditions in their extended outer envelopes. It also bears on the issue of late-type dwarfs orbiting main sequence B stars, the evolutionary predecessors of K bright giants. We propose to directly image the putative hybrid companions using Chandra, with supporting observations from HST/WFPC2.

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