Evaluating the Role of Photoevaporation in Protoplanetary Disk Dispersal

Details Evaluating the Role of Photoevaporation in Protoplanetary Disk Dispersal Evaluating the Role of Photoevaporation in Protoplanetary Disk Dispersal

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2308h&link_type=abstract

Chandra Proposal ID #09200905

Physics

Chandra Proposal Id #09200905

Scientific paper

Emission produced by accretion onto the central star leads to photoevaporation, which may play a fundamental role in disk dispersal. Models of disk photoevaporation by the central star are challenged by two potential problems: the emission produced by accretion will be substantially weaker for low-mass stars, and photoevaporation must continue as accretion slows. We propose use HST/ACS SBC PR130L to obtain FUV spectra of WTTSs and of CTTSs at low masses and mass accretion rates to provide crucial data to evaluate photoevaporation models. We will estimate the FUV and EUV luminosities of low-mass CTTSs with small mass accretion rates, CTTSs with transition disks and slowed accretion, and of magnetically-active WTTSs.

Affiliated with

Also associated with

No associations

Rating

Evaluating the Role of Photoevaporation in Protoplanetary Disk Dispersal 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 Evaluating the Role of Photoevaporation in Protoplanetary Disk Dispersal, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evaluating the Role of Photoevaporation in Protoplanetary Disk Dispersal will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-964326