A deep UV imaging survey of the Globular Cluster M 30

Details A deep UV imaging survey of the Globular Cluster M 30 A deep UV imaging survey of the Globular Cluster M 30

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hst..prop10561d&link_type=abstract

HST Proposal ID #10561

Physics

Hst Proposal Id #10561 Hot Stars

Scientific paper

We propose to carry out a deep FUV and NUV survey of M30 {NGC 7099} in order to find and study the hot and/or dynamically-formed stellar populations in the globular cluster. In particular, we will {i} search for the UV counterpart to a MSP binary, {ii} find and study the full population of cataclysmic variables in this cluster, {iii} study the UV properties of the cluster's extensive blue straggler population, {iv} detect the first set of white dwarfs in this cluster. Our survey will be sensitive to variability on time-scales from minutes to weeks, allowing us to search for variable stars in all of the FUV populations.

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