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Abundance analysis in the near IR: stellar clusters and galaxies

Abundance analysis in the near IR: stellar clusters and galaxies

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_807264890

Abundance analysis in the near IR: stellar clusters and galaxies

About this item

Full title

Abundance analysis in the near IR: stellar clusters and galaxies

Author / Creator

Publisher

Dordrecht: Springer Nature B.V

Journal title

Astrophysics and space science, 2001-05, Vol.277 (1), p.177-180

Language

English

Formats

Publication information

Publisher

Dordrecht: Springer Nature B.V

More information

Scope and Contents

Contents

Massive red supergiants and low mass giants with typical temperatures in the range3000-5000 K can dominate the infrared (IR) luminosity of integrated stellar systems. The near IR spectra of these stars show many absorption lines due to neutral metals and molecules like CO and OH.A reasonable number of these lines can be be measured also at relative...

Alternative Titles

Full title

Abundance analysis in the near IR: stellar clusters and galaxies

Authors, Artists and Contributors

Author / Creator

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_807264890

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_807264890

Other Identifiers

ISSN

0004-640X

E-ISSN

1572-946X

DOI

10.1023/A:1012701726947

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