Veiling in Orion T Tauri Stars

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We use the cross dispersed echelle spectrometer on the 2.7 m Harlan J. Smith telescope at McDonald Observatory to measure the optical veiling in several classical T Tauri stars with known rotation periods in the Orion star formation region. Veiling is the excess continuum produced as circumstellar matter accretes onto the stellar surface. Pervious studies have generally ignored this excess continuum when analyzing the V, R and I colors to determine stellar and accretion properties of the low mass young stars in Orion. We find for a number of stars that the veiling flux contributes significantly to the V and Ic colors. We use our veiling measurements to correct literature photometric data in order to calculate new extinction values and intrinsic magnitudes for each star. We then use these corrected magnitudes with pre-main sequence evolutionary tracks to obtain new estimates of the stellar luminosity, radius, mass, and age of each star in our sample. Combining these updated parameters with our veiling measurements, we determine accurate accretion rate estimates which we will use to test disk locking theory in the low mass stars of Orion. This research was supported in part by a NASA Origins grant to Rice University.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Veiling in Orion T Tauri 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 Veiling in Orion T Tauri Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Veiling in Orion T Tauri Stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1281599

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.