The spectra of late type dwarfs and sub-dwarfs in the near ultraviolet. II - Limits to variability in MgII emission from IUE spectrophotometry

Details The spectra of late type dwarfs and sub-dwarfs in the near ultraviolet. II - Limits to variability in MgII emission from IUE spectrophotometry The spectra of late type dwarfs and sub-dwarfs in the near ultraviolet. II - Limits to variability in MgII emission from IUE spectrophotometry

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...52..135c&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 52, April 1983, p. 135-142. Research supported by the Consig

Astronomy and Astrophysics

Astrophysics

14

Dwarf Stars, G Stars, Iue, Late Stars, Stellar Spectra, Stellar Spectrophotometry, Ultraviolet Spectra, Chromosphere, Data Reduction, Emission Spectra, Line Spectra, Magnesium, Subdwarf Stars

Scientific paper

The chromospheric h and k emission cores of the G dwarfs and subdwarfs Beta Hyi (14), Zeta Tuc (5), Delta Pav (5), and Tau Cet (5) have been monitored over a period of four years using the IUE satellite long wavelength camera. A detailed statistical examination of the data has shown that no variation in h and k fluxes of less than 15 percent could have been detected by means of this technique. This limit applies, even after removing the effects of saturation, variable gain, and scattered light between echelle orders, for any astrophysical use of comparable IUE data. No flux excursions larger than this value were detected in any of the objects presently considered.

Affiliated with

Also associated with

No associations

Rating

The spectra of late type dwarfs and sub-dwarfs in the near ultraviolet. II - Limits to variability in MgII emission from IUE spectrophotometry 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 spectra of late type dwarfs and sub-dwarfs in the near ultraviolet. II - Limits to variability in MgII emission from IUE spectrophotometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectra of late type dwarfs and sub-dwarfs in the near ultraviolet. II - Limits to variability in MgII emission from IUE spectrophotometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1233114