The Impact of Accurate Distances on UV Spectroscopy of White Dwarfs and Cataclysmic Variables

Details The Impact of Accurate Distances on UV Spectroscopy of White Dwarfs and Cataclysmic Variables The Impact of Accurate Distances on UV Spectroscopy of White Dwarfs and Cataclysmic Variables

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1135..291b&link_type=abstract

FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic

Computer Science

Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Photometric, Polarimetric, And Spectroscopic Instrumentation, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

J-MAPS and Gaia are two asterometry missions to be launched in 2012. The positions of stars brighter than 15 magnitude will be measured to accuracies of better than one milli-arcsecond and 25 micro-arcseconds, respectively. Accurate distances (3 hr) and gravitational braking for those below the gap (<2 hr). For nova-like systems, whose luminosity is dominated by the accretion disk and affected by interstellar extinction and reddening, accurate distances can help constrain the temperature profile of the disk.

Affiliated with

Also associated with

No associations

Rating

The Impact of Accurate Distances on UV Spectroscopy of White Dwarfs and Cataclysmic Variables does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Impact of Accurate Distances on UV Spectroscopy of White Dwarfs and Cataclysmic Variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Impact of Accurate Distances on UV Spectroscopy of White Dwarfs and Cataclysmic Variables will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1111864