Sizes of Masing Parts of Massive Star Forming Regions
It is shown that the images, line profiles, and time evolution of different interstellar masing transitions can be explained by the hypothesis that the population inversions giving birth to masers take place in turbulent regions with extents that are orders of magnitude greater than the sizes of the...
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| Date: | 2012 |
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| Language: | rus |
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Видавничий дім «Академперіодика»
2012
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| Online Access: | http://rpra-journal.org.ua/index.php/ra/article/view/550 |
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| Journal Title: | Radio physics and radio astronomy |
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oai:ri.kharkov.ua:article-5502012-12-09T20:56:27Z Sizes of Masing Parts of Massive Star Forming Regions Sizes of Masing Parts of Massive Star Forming Regions Sobolev, A. M. Sutton, E. C. Watson, W. D. Ostrovskii, A. B. Shelemei, O. V. It is shown that the images, line profiles, and time evolution of different interstellar masing transitions can be explained by the hypothesis that the population inversions giving birth to masers take place in turbulent regions with extents that are orders of magnitude greater than the sizes of the maser spots. It is shown that the images of methanol masers in the turbulent model persist within considerable time and do not prevent measurement of the annual parallaxes using data on the 12 GHz methanol maser positions. It is shown that the images, line profiles, and time evolution of different interstellar masing transitions can be explained by the hypothesis that the population inversions giving birth to masers take place in turbulent regions with extents that are orders of magnitude greater than the sizes of the maser spots. It is shown that the images of methanol masers in the turbulent model persist within considerable time and do not prevent measurement of the annual parallaxes using data on the 12 GHz methanol maser positions. Видавничий дім «Академперіодика» 2012-12-09 Article Article application/pdf http://rpra-journal.org.ua/index.php/ra/article/view/550 РАДИОФИЗИКА И РАДИОАСТРОНОМИЯ; Vol 13, No 3 (2008); 76 RADIO PHYSICS AND RADIO ASTRONOMY; Vol 13, No 3 (2008); 76 РАДІОФІЗИКА І РАДІОАСТРОНОМІЯ; Vol 13, No 3 (2008); 76 2415-7007 1027-9636 rus http://rpra-journal.org.ua/index.php/ra/article/view/550/124 |
| institution |
Radio physics and radio astronomy |
| baseUrl_str |
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| datestamp_date |
2012-12-09T20:56:27Z |
| collection |
OJS |
| language |
rus |
| format |
Article |
| author |
Sobolev, A. M. Sutton, E. C. Watson, W. D. Ostrovskii, A. B. Shelemei, O. V. |
| spellingShingle |
Sobolev, A. M. Sutton, E. C. Watson, W. D. Ostrovskii, A. B. Shelemei, O. V. Sizes of Masing Parts of Massive Star Forming Regions |
| author_facet |
Sobolev, A. M. Sutton, E. C. Watson, W. D. Ostrovskii, A. B. Shelemei, O. V. |
| author_sort |
Sobolev, A. M. |
| title |
Sizes of Masing Parts of Massive Star Forming Regions |
| title_short |
Sizes of Masing Parts of Massive Star Forming Regions |
| title_full |
Sizes of Masing Parts of Massive Star Forming Regions |
| title_fullStr |
Sizes of Masing Parts of Massive Star Forming Regions |
| title_full_unstemmed |
Sizes of Masing Parts of Massive Star Forming Regions |
| title_sort |
sizes of masing parts of massive star forming regions |
| title_alt |
Sizes of Masing Parts of Massive Star Forming Regions |
| description |
It is shown that the images, line profiles, and time evolution of different interstellar masing transitions can be explained by the hypothesis that the population inversions giving birth to masers take place in turbulent regions with extents that are orders of magnitude greater than the sizes of the maser spots. It is shown that the images of methanol masers in the turbulent model persist within considerable time and do not prevent measurement of the annual parallaxes using data on the 12 GHz methanol maser positions. |
| publisher |
Видавничий дім «Академперіодика» |
| publishDate |
2012 |
| url |
http://rpra-journal.org.ua/index.php/ra/article/view/550 |
| work_keys_str_mv |
AT sobolevam sizesofmasingpartsofmassivestarformingregions AT suttonec sizesofmasingpartsofmassivestarformingregions AT watsonwd sizesofmasingpartsofmassivestarformingregions AT ostrovskiiab sizesofmasingpartsofmassivestarformingregions AT shelemeiov sizesofmasingpartsofmassivestarformingregions |
| first_indexed |
2025-07-17T11:34:02Z |
| last_indexed |
2025-07-17T11:34:02Z |
| _version_ |
1837893726303682560 |