Ranking line-depth ratios for determining relative star temperatures in dwarfs
The central line-depths of absorption lines depend upon stellar temperature. By dividing the central line-depth of such a line with a central line-depth independent of temperature, a thermometer of relative star temperatures is obtained in the form of a line-depth ratio (LDR), once it is related to...
Main Author: | Edstam, Louise |
---|---|
Format: | Others |
Language: | English |
Published: |
Uppsala universitet, Observationell astrofysik
2013
|
Subjects: | |
Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-202315 |
Similar Items
-
THE CHROMOSPHERES OF M DWARF STARS
by: Giampapa, M. S. (Mark S.)
Published: (1980) -
A gravitational redshift determination of the mean mass of white dwarfs. DA stars.
by: Falcon, Ross Edward
Published: (2010) -
On the reliability of 2MASS data in identifying red dwarf stars
by: Snyder, Lucas A.
Published: (2011) -
Spectroscopic properties of granulation in K-type dwarf stars
by: Ramírez, Iván, 1979-
Published: (2008) -
Spectroscopic and photometric studies of main sequence M stars and a search for late-type dwarfs in the solar vicinity.
by: Kirkpatrick, Joseph Davy.
Published: (1992)