Other
Scientific paper
Oct 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..134a&link_type=abstract
XMM-Newton Proposal ID #05035505
Other
Stars, White Dwarfs, Solar System, Rxs J093119.2+3, Rxs J163421.8+3, Rxs 120428.0+58, Rxs J101340.6+0, Rxs J153221.7+4, Xmm-Newton Proposal 05035505
Scientific paper
Among the ~6000 new white dwarfs (WDs) spectroscopically confirmed by the Sloan Digital Sky Survey (SDSS) are three cool DAs and two cool DBs within 1 of super-soft ROSAT All Sky Survey (RASS) sources. WDs at these relatively low temperatures (<23,000K) are not expected to be X-ray emitters, but the SDSS photometric and spectroscopic data fail to identify any other obvious optical counterparts to the RASS sources to the SDSS limits (g~23 mag in photometry). We propose 5 ksec XMM-Newton observations of these five SDSS WDs to obtain pinpoint X-ray positions and improved flux measures for these objects. If XMM data confirm that the five WDs are X-ray sources, they will be of great interest; in particular, theoretical work will be required to explain how such cool WDs can emit X rays.
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