The ultraviolet spectrum of solar analogs

Details The ultraviolet spectrum of solar analogs The ultraviolet spectrum of solar analogs

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..332a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 332-342. Research supported by MPI.

Astronomy and Astrophysics

Astrophysics

5

Line Spectra, Stellar Radiation, Sun, Ultraviolet Spectra, Chromosphere, High Resolution, Iron, Magnesium, Photosphere

Scientific paper

The ultraviolet high resolution IUE spectrum between 2600 and 3200 A of a sample of stars classified as solar analogs by Hardorp (1982 and references therein), including the southern solar twin HR 2290, is studied. A list of Fe II absorption line identifications and equivalent widths in the considered spectral region is presented. An analysis of the Mg II 2800 A emission doublet and of the Fe II absorption spectrum is performed and the results are discussed in terms of Hardorp's solar analogy class. It turns out that, while the Hardorp-class-1 analog (HR 2290) shows chromospheric Mg II and photospheric Fe II features close to the sun, for the other analogy classes no direct correspondence seems to exist either with the Mg II emission or with the Fe II absorption spectrum.

Affiliated with

Also associated with

No associations

Rating

The ultraviolet spectrum of solar analogs 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 ultraviolet spectrum of solar analogs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The ultraviolet spectrum of solar analogs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1123952