Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..107d&link_type=abstract
In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 107-110 (SEE N85-20961 1
Astronomy and Astrophysics
Astronomy
8
Carbon, Galactic Evolution, Interstellar Matter, Iue, Nitrogen, Oxygen, Ultraviolet Astronomy, Chemical Composition, H Ii Regions, Magellanic Clouds, Mathematical Models, Nebulae, Nuclear Fusion
Scientific paper
During the last several years IUE observations of UV spectra of galactic and extragalactic H II regions have provided the first good quantitative measurements of gaseous-phase C abundances in the ISM of several galaxies over a broad range of "metallicity". This paper illustrates the observed relative variations of C, N, and O based on IUE and ground-based observations of H II regions and discusses the trends evident using current concepts regarding stellar nucleosynthesis of CNO element group and simple models of galactic chemical evolution.
No associations
LandOfFree
Comments on the origins and variations of carbon and nitrogen in the ISM of galaxies as evident from IUE spectroscopy of H 2 regions 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 Comments on the origins and variations of carbon and nitrogen in the ISM of galaxies as evident from IUE spectroscopy of H 2 regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comments on the origins and variations of carbon and nitrogen in the ISM of galaxies as evident from IUE spectroscopy of H 2 regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-738233