Published December 1990 | Version v1
Journal article Metadata-only

Equivalent widths for Fe-group lines in field and cluster metal poor stars

Creators

  • 1. Osservatorio Astronomico Padova, (Italy)
  • 2. Texas Univ., Austin, TX (USA). Dept. of Astronomy

Description

Abundances of Fe-group elements in field and cluster metal poor stars have been presented in Gratton and Sneden (1990). Here we present a tabulation of the equivalent widths used in that paper. Errors in these equivalent widths are ±2m A for field stars, and ±10m A in cluster giants. These errors are mainly due to uncertainties (∼ 1/1.5%) in the location of the continuum level

Additional details

Publishing Information

Journal Title
Astronomy and Astrophysics, Supplement Series
Journal Volume
86
Journal Issue
2
Series
Astron. Astrophys., Suppl. Ser.
Journal Page Range
269-298
ISSN
0365-0138
CODEN
AAESB

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
22036052
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ELEMENT ABUNDANCE; GIANT STARS; IRON; SPECTRA; STAR CLUSTERS
Descriptors DEC
ELEMENTS; METALS; QUANTITY RATIO; STARS; TRANSITION ELEMENTS