Systematic Effects and a New Determination of the Primordial Abundance of4He anddY/dZfrom Observations of Blue Compact Galaxies
Author(s) -
Y. I. Izotov,
T. X. Thuan
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/380830
Subject(s) - physics , metallicity , astrophysics , nucleosynthesis , galaxy , analytical chemistry (journal) , big bang nucleosynthesis , excited state , mass fraction , linear regression , atomic physics , stars , chemistry , statistics , chromatography , thermodynamics , mathematics
We use spectroscopic observations of a sample of 82 HII regions in 76 bluecompact galaxies to determine the primordial helium abundance Yp and the slopedY/dZ from the Y-O/H linear regression. To improve the accuracy of the dY/dZmeasurement, we have included new spectrophotometric observations of 33 HIIregions which span a large metallicity range, with oxygen abundance 12+log(O/H)varying between 7.43 and 8.30 (Zsun/30
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom