Physics
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1917c&link_type=abstract
Chandra Proposal ID #07400020
Physics
Chandra Proposal Id #07400020
Scientific paper
He-rich thermonuclear bursts are at present unexamined by high-sensitivity, high-spectral resolution observations. Theoretical simulations predict conditions at the peak of such bursts conducive to producing rich emission line spectra from a range of heavy elements. We propose observations of 4U 1728-34, the only source which produces frequent He-rich bursts, in order to test for such lines and also to undertake a deep search for peristent spectral features and orbital intensity modulations.
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