COS-GTO: Activity of Solar Mass Stars from Cradle to Grave

Details COS-GTO: Activity of Solar Mass Stars from Cradle to Grave COS-GTO: Activity of Solar Mass Stars from Cradle to Grave

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11532g&link_type=abstract

HST Proposal ID #11532. Cycle 17

Physics

Scientific paper

COS spectra will be very useful for answering the question of how chromospheric and coronal activity of stars decline as stars lose angular momentum and magnetic fields with age. This question is important for modelling the atmospheres of young planets that are blasted by strong ultraviolet radiation and winds from young stars. COS will obtain spectra of solar mass stars with a range of ages from 10 Myr to 7 Gyr.;

Affiliated with

Also associated with

No associations

Rating

COS-GTO: Activity of Solar Mass Stars from Cradle to Grave 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 COS-GTO: Activity of Solar Mass Stars from Cradle to Grave, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and COS-GTO: Activity of Solar Mass Stars from Cradle to Grave will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1320138