The Interstellar Medium in Galaxies:
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Dordrecht
Springer Netherlands
1997
|
| Series: | Astrophysics and Space Science Library
219 |
| Subjects: | |
| Online Access: | Volltext |
| Item Description: | It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an "outside" view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way |
| Physical Description: | 1 Online-Ressource (X, 212 p) |
| ISBN: | 9789401156202 9781402003790 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-011-5620-2 |
Staff View
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| 500 | |a It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an "outside" view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way | ||
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| id | DE-604.BV042416078 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:59Z |
| institution | BVB |
| isbn | 9789401156202 9781402003790 |
| issn | 0067-0057 |
| language | English |
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| spelling | Hulst, J. M. Verfasser aut The Interstellar Medium in Galaxies edited by J. M. Hulst Dordrecht Springer Netherlands 1997 1 Online-Ressource (X, 212 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library 219 0067-0057 It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an "outside" view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way Physics Astronomy, Observations and Techniques Interstellare Materie (DE-588)4162140-2 gnd rswk-swf Interstellare Materie (DE-588)4162140-2 s 1\p DE-604 https://doi.org/10.1007/978-94-011-5620-2 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Hulst, J. M. The Interstellar Medium in Galaxies Physics Astronomy, Observations and Techniques Interstellare Materie (DE-588)4162140-2 gnd |
| subject_GND | (DE-588)4162140-2 |
| title | The Interstellar Medium in Galaxies |
| title_auth | The Interstellar Medium in Galaxies |
| title_exact_search | The Interstellar Medium in Galaxies |
| title_full | The Interstellar Medium in Galaxies edited by J. M. Hulst |
| title_fullStr | The Interstellar Medium in Galaxies edited by J. M. Hulst |
| title_full_unstemmed | The Interstellar Medium in Galaxies edited by J. M. Hulst |
| title_short | The Interstellar Medium in Galaxies |
| title_sort | the interstellar medium in galaxies |
| topic | Physics Astronomy, Observations and Techniques Interstellare Materie (DE-588)4162140-2 gnd |
| topic_facet | Physics Astronomy, Observations and Techniques Interstellare Materie |
| url | https://doi.org/10.1007/978-94-011-5620-2 |
| work_keys_str_mv | AT hulstjm theinterstellarmediumingalaxies |