Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-06
Astrophys.Space Sci. 277 (2001) 545-563
Astronomy and Astrophysics
Astrophysics
16 pages, 3 postscript (EPS) figures, TEX, uses psfig.sty, to be published in Astrophysics and Space Science, also available a
Scientific paper
10.1023/A:1013827617446
In this work, two aspects of the chemical evolution of 4He in the Galaxy are considered on the basis of a sample of disk planetary nebulae (PN). First, an application of corrections owing to the contamination of 4He from the evolution of the progenitor stars shows that the He/H abundance by number of atoms is reduced by 0.012 to 0.015 in average, leading to an essentially flat He/H radial distribution. Second, a determination of the helium to heavy element enrichment ratio using the same corrections leads to values in the range 2.8 < Delta Y/Delta Z < 3.6 for Yp = 0.23 and 2.0 < Delta Y/Delta Z < 2.8 for Yp = 0.24, in good agreement with recent independent determinations and theoretical models.
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