Class I methanol maser emission in infrared clouds and the third version of the Astro Space Center MMI/SFR catalog

OS Bayandina, IE Val'tts, GM Larionov - Astronomy reports, 2012 - Springer
OS Bayandina, IE Val'tts, GM Larionov
Astronomy reports, 2012Springer
We have revised the Astro Space Center catalog of Class I methanol masers detected in star-
forming regions (MMI/SFR), mainly at 44 GHz, and created a new electronic version of the
catalog. Currently, the catalog contains 206 objects, selected from publications through
2011 inclusive. The data from the survey of Chen et al.(2011), performed specifically for
objects EGO, which form a new specific catalog, are not included. The MMI/SFR objects
were identified with emission and absorption objects in the near IR, detected during the MSX …
Abstract
We have revised the Astro Space Center catalog of Class I methanol masers detected in star-forming regions (MMI/SFR), mainly at 44 GHz, and created a new electronic version of the catalog. Currently, the catalog contains 206 objects, selected from publications through 2011 inclusive. The data from the survey of Chen et al. (2011), performed specifically for objects EGO, which form a new specific catalog, are not included. The MMI/SFR objects were identified with emission and absorption objects in the near IR, detected during the MSX and Spitzer space missions. Seventy-one percent of Class I methanol masers that emit at 44 GHz and fall within the Galactic longitude range surveyed by Spitzer (GLIMPSE) are identified with Spitzer Dark Clouds (SDCs), and 42% with Extended Green Objects (EGOs). It is possible that Class I methanol masers arise in isolated, self-gravitating clumps, such as SDCs, at certain stages of their evolution. A sample of SDCs is proposed as a new target list for Class I methanol maser searches. A detailed statistical analysis was carried out, taking into account the characteristics of the regions of MMI/SFR formation presented in the catalog.
Springer
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