Models for the active and quiescent regions on the RS CVN-type system 2 Pegasi (HD 224085)

Details Models for the active and quiescent regions on the RS CVN-type system 2 Pegasi (HD 224085) Models for the active and quiescent regions on the RS CVN-type system 2 Pegasi (HD 224085)

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..351l&link_type=abstract

In ESA Fourth European IUE Conf. p 351-354 (SEE N84-35135 24-88)

Computer Science

5

Binary Stars, Data Acquisition, Stellar Atmospheres, Stellar Models, Data Correlation, Electron Density Profiles, Faculae, Iue, Radiative Transfer

Scientific paper

The IUE observations of the RS CVn binary system II Pegasi obtained during the period 1981 October 1-7 were used to derive the emission measure distributions and to calculate transmission region models of the quiescent and plage (active) regions of II Peg. Active region models were calculated assuming area coverages of 10%, 6%, 3% and 1% of the visible hemisphere. These models are used to provide lower limits to the electron pressure in the quiescent and plage regions, which are compared with the available density diagnostics. The amount of mechanical energy deposition required to account for the observed radiative losses is very large.

Affiliated with

Also associated with

No associations

Rating

Models for the active and quiescent regions on the RS CVN-type system 2 Pegasi (HD 224085) 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 Models for the active and quiescent regions on the RS CVN-type system 2 Pegasi (HD 224085), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models for the active and quiescent regions on the RS CVN-type system 2 Pegasi (HD 224085) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1705905