CS observations of selected star-forming regions
| ISSN: |
1572-946X
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|---|---|
| Source: |
Springer Online Journal Archives 1860-2000
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| Topics: |
Physics
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| Notes: |
Abstract Maps of the CS (J=1→0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, our observations show evidence of some remarkable morphological differences.
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798296447331860480 |
|---|---|
| autor | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. |
| autorsonst | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. |
| book_url | http://dx.doi.org/10.1007/BF00646374 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLM193033372 |
| issn | 1572-946X |
| journal_name | Astrophysics and space science |
| materialart | 1 |
| notes | Abstract Maps of the CS (J=1→0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, our observations show evidence of some remarkable morphological differences. |
| package_name | Springer |
| publikationsjahr_anzeige | 1989 |
| publikationsjahr_facette | 1989 |
| publikationsjahr_intervall | 8014:1985-1989 |
| publikationsjahr_sort | 1989 |
| publisher | Springer |
| reference | 156 (1989), S. 251-256 |
| search_space | articles |
| shingle_author_1 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. |
| shingle_author_2 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. |
| shingle_author_3 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. |
| shingle_author_4 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. |
| shingle_catch_all_1 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. CS observations of selected star-forming regions Abstract Maps of the CS (J=1→0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, our observations show evidence of some remarkable morphological differences. 1572-946X 1572946X Springer |
| shingle_catch_all_2 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. CS observations of selected star-forming regions Abstract Maps of the CS (J=1→0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, our observations show evidence of some remarkable morphological differences. 1572-946X 1572946X Springer |
| shingle_catch_all_3 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. CS observations of selected star-forming regions Abstract Maps of the CS (J=1→0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, our observations show evidence of some remarkable morphological differences. 1572-946X 1572946X Springer |
| shingle_catch_all_4 | Buj, J. Estalella, R. López, R. Anglada, G. Planesas, P. CS observations of selected star-forming regions Abstract Maps of the CS (J=1→0) emission at 49 GHz of L43 (RNO 91), NGC 2068 (HH 19-27) and L1524 (Haro 6-10) are presented. Physical parameters of these clouds are derived from the observations. The CS emission is compared with ammonia emission maps obtained with a similar angular resolution. Both CS and ammonia molecules are tracers of the high-density gas in molecular clouds. Thus, a similar distribution of the emission is expected. However, our observations show evidence of some remarkable morphological differences. 1572-946X 1572946X Springer |
| shingle_title_1 | CS observations of selected star-forming regions |
| shingle_title_2 | CS observations of selected star-forming regions |
| shingle_title_3 | CS observations of selected star-forming regions |
| shingle_title_4 | CS observations of selected star-forming regions |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Springer Online Journal Archives 1860-2000 |
| timestamp | 2024-05-06T09:52:15.071Z |
| titel | CS observations of selected star-forming regions |
| titel_suche | CS observations of selected star-forming regions |
| topic | U |
| uid | nat_lic_papers_NLM193033372 |