Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sci...291...93b&link_type=abstract
Science, Volume 291, Issue 5501, pp. 93-97 (2001).
Astronomy and Astrophysics
Astronomy
85
Scientific paper
We are conducting a large-scale, multiepoch, optical photometric survey [Centro de Investigaciones de Astronomía-Quasar Equatorial Survey Team (CIDA-QUEST)] covering about 120 square degrees to identify the young low-mass stars in the Orion OB1 association. We present results for an area of 34 square degrees. Using photometric variability as our main selection criterion, as well as follow-up spectroscopy, we confirmed 168 previously unidentified pre-main sequence stars that are about 0.6 to 0.9 times the mass of the sun (Msolar), with ages of about 1 million to 3 million years (Ori OB1b) and about 3 million to 10 million years (Ori OB1a). The low-mass stars are spatially coincident with the high-mass (at least 3 Msolar) members of the associations. Indicators of disk accretion such as Hα emission and near-infrared emission from dusty disks fall sharply from Ori OB1b to Ori OB1a, indicating that the time scale for disk dissipation and possibly the onset of planet formation is a few million years.
Andrews Peter
Berlind Perry
Briceno Cesar
Calvet Nuria
Hartmann Lee
No associations
LandOfFree
The CIDA-QUEST Large-Scale Survey of Orion OB1: Evidence for Rapid Disk Dissipation in a Dispersed Stellar Population 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 CIDA-QUEST Large-Scale Survey of Orion OB1: Evidence for Rapid Disk Dissipation in a Dispersed Stellar Population, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The CIDA-QUEST Large-Scale Survey of Orion OB1: Evidence for Rapid Disk Dissipation in a Dispersed Stellar Population will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-905059