COS-GTO: Accretion Flows and Winds of Pre-Main Sequence Stars

Details COS-GTO: Accretion Flows and Winds of Pre-Main Sequence Stars COS-GTO: Accretion Flows and Winds of Pre-Main Sequence Stars

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11533g&link_type=abstract

HST Proposal ID #11533. Cycle 17

Physics

Scientific paper

COS will obtain spectra of T Tauri stars to study accretion flows and wind absorption features in ultraviolet emission lines. Observations of several T Tauri stars with different inclination angles with respect to the line of sight will determine the temperature distributions, flow velocities, and column densities of both inflows and outflows for these stars.;

Affiliated with

Also associated with

No associations

Rating

COS-GTO: Accretion Flows and Winds of Pre-Main Sequence Stars 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: Accretion Flows and Winds of Pre-Main Sequence Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and COS-GTO: Accretion Flows and Winds of Pre-Main Sequence Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1320139