Published May 9, 2014
| Version v1
Journal article
Abundance measurements in stellar environments
Creators
- 1. Università di Catania, Dipartimento di Fisica e Astronomia, Sezione Astrofisica, Via S. Sofia 78, 95123 Catania (Italy)
Description
Most of what we know about stars, and systems of stars, is derived from the analysis of their electromagnetic radiation. This lesson is an attempt to describe to Physicists, without any Astrophysical background, the framework to understand the present status of abundance determination in stellar environments and its limit. These notes are dedicated to the recently passed, November 21, 2013, Prof. Dimitri Mihalas who spent his life confuting the 19th century positivist philosopher Auguste Comte who stated that we shall not at all be able to determine the chemical composition of stars
Additional details
Identifiers
- DOI
- 10.1063/1.4875292;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1595
- Journal Issue
- 1
- Journal Page Range
- p. 69-75
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 7. European summer school on experimental nuclear astrophysics
- Dates
- 15-17 Sep 2013
- Place
- Santa Tecla, Sicily (Italy)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 45101771
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; CHEMICAL COMPOSITION; ELECTROMAGNETIC RADIATION; ELEMENT ABUNDANCE; STARS
- Descriptors DEC
- ABUNDANCE; PHYSICS; RADIATIONS
Optional Information
- Notes
- (c) 2014 AIP Publishing LLC