Molecular diagnostics of the interstellar medium and star forming regions
Astrophysics and Space Science, ISSN: 0004-640X, Vol: 237, Issue: 1-2, Page: 267-298
1996
- 2Citations
- 5Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Article Description
Selected examples of the use of observationally inferred molecular level populations and chemical compositions in the diagnosis of interstellar sources and processes important in them (and in other diffuse astrophysical sources) are given. The sources considered include the interclump medium of a giant molecular cloud, dark cores which are the progenitors of star formation, material responding to recent star formation and which may form further stars, and stellar ejecta (including those of supernovae) about to merge with the interstellar medium. The measurement of the microwave background, mixing of material between different nuclear burning zones in evolved stars and turbulent boundary layers (which are present in and influence the structures and evolution of all diffuse astrophysical sources) are treated.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=0347245204&origin=inward; http://dx.doi.org/10.1007/bf02424435; http://link.springer.com/10.1007/BF02424435; http://link.springer.com/content/pdf/10.1007/BF02424435.pdf; http://www.springerlink.com/index/pdf/10.1007/BF02424435; http://www.springerlink.com/index/10.1007/BF02424435; https://dx.doi.org/10.1007/bf02424435; https://link.springer.com/article/10.1007/BF02424435
Springer Nature
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