Dynamics and Energy Balance in Stellar Transition Regions - Repeat for HOPR#66

Details Dynamics and Energy Balance in Stellar Transition Regions - Repeat for HOPR#66 Dynamics and Energy Balance in Stellar Transition Regions - Repeat for HOPR#66

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.4768l&link_type=abstract

HST Proposal ID #4768

Astronomy and Astrophysics

Astrophysics

Hst Proposal Id #4768 Stellar Astrophysics

Scientific paper

We propose to study the dynamics of stellar transition regions by measuring the redshifts, indicative of downflows, in lines of C III, C IV, Si IV, and O IV.The energy balance and heating rates in stellar chromospheres and transition regions will be derived from an emission measure analysis of emission line fluxes and densities inferred from density sensitive line ratios. Stars of interest include dwarf stars of spectral type F-M, active G and K giants, and RS CVn binary systems.

Affiliated with

Also associated with

No associations

Rating

Dynamics and Energy Balance in Stellar Transition Regions - Repeat for HOPR#66 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 Dynamics and Energy Balance in Stellar Transition Regions - Repeat for HOPR#66, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics and Energy Balance in Stellar Transition Regions - Repeat for HOPR#66 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862767