Ultraviolet Study of the Chamaeleon T-Association

Details Ultraviolet Study of the Chamaeleon T-Association Ultraviolet Study of the Chamaeleon T-Association

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1843l&link_type=abstract

IUE Proposal ID #LDGJL

Other

Scientific paper

The Chamaeleon T1 association is a nearby compact star-forming region which has been extensively studied at optical, infrared and X-ray wavelengths. We propose to observe the brightest pre-main sequence stars in this association with IUE. SWP low dispersion and LWP low and high dispersion spectra would be obtained for these stars which have formed essentially coevally (within the free-fall collapse time of the single cloud from which they originate). Their chromospheric and coronal properties will be studied using emission measure modelling techniques based on these IUE spectra and -the extensive database from other spectral regions. The derived properties of -the outer atmospheres will be investigated in relation to the general propertie's of the stars, particularly position in the HR diagram, mass loss rate and stellar mass. Detailed comparison of apparently similar stars from different star formation regions will be made.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet Study of the Chamaeleon T-Association 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 Ultraviolet Study of the Chamaeleon T-Association, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet Study of the Chamaeleon T-Association will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1707109