2025-02-23T13:42:45-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-8413%22&qt=morelikethis&rows=5
2025-02-23T13:42:45-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-8413%22&qt=morelikethis&rows=5
2025-02-23T13:42:45-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-23T13:42:45-05:00 DEBUG: Deserialized SOLR response
Sizes of Masing Parts of Massive Star Forming Regions

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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Bibliographic Details
Main Authors: Sobolev, A.M., Sutton, E.C., Watson, W.D., Ostrovskii, A.B., Shelemei, O.V.
Format: Article
Language:English
Published: Радіоастрономічний інститут НАН України 2008
Subjects:
Астрофизика
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/8413
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2025-02-23T13:42:45-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&rows=40&rows=5&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-8413%22&qt=morelikethis
2025-02-23T13:42:45-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&rows=40&rows=5&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-8413%22&qt=morelikethis
2025-02-23T13:42:45-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-23T13:42:45-05:00 DEBUG: Deserialized SOLR response

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