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Items where Person is "Heithausen-A"

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Jump to: 2004 | 2003 | 1997
Number of items: 6.

2004

Lis, D. C. and Gerin, M. and Roueff, E. et al. (2004) Deuterated Species in Star-Forming Regions. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer , Berlin, pp. 487-490. ISBN 978-3-642-62348-6. https://resolver.caltech.edu/CaltechAUTHORS:20171127-153159871

Comito, C. and Schilke, P. and Gerin, M. et al. (2004) The Line-of-Sight Distribution of Water in SgrB2. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer Berlin Heidelberg , Berlin, Heidelberg, pp. 265-268. ISBN 9783642623486. https://resolver.caltech.edu/CaltechAUTHORS:20190826-124739891

2003

Bradford, C. M. and Zmuidzinas, J. (2003) The Future of Far-IR/Submillimeter Astrophysics with Single Dish Telescopes. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer Berlin Heidelberg , Berlin, Heidelberg, pp. 323-330. ISBN 9783642623486. https://resolver.caltech.edu/CaltechAUTHORS:20190826-124739989

1997

Hillenbrand, L. A. (1997) Mass Function of Newly Formed Stars. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer , Berlin, pp. 601-609. ISBN 978-3-642-62348-6. https://resolver.caltech.edu/CaltechAUTHORS:20200610-082408943

Chapman, S. C. and Blain, A. and Ivison, R. et al. (1997) A Spectroscopic Survey of the Submillimeter Galaxy Population: 85 Redshifts Using Keck/LRIS-B. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer , Berlin, pp. 15-21. ISBN 978-3-642-62348-6. https://resolver.caltech.edu/CaltechAUTHORS:20200325-142553056

Houde, M. and Phillips, T. G. and Hildebrand, R. H. et al. (1997) Tracing the Magnetic Field in Molecular Clouds. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer , Berlin, pp. 365-368. ISBN 978-3-642-62348-6. https://resolver.caltech.edu/CaltechAUTHORS:20200221-090156145

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