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Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment
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title
Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment
Creator
Daniel Tafoya, †
De La Fuente, Eduardo
Franco, José
Kemp, Simon
Kurtz, Stanley
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ArXiv
abstract
The Karl Jansky Very Large Array (VLA), Owens Valley Radio Observatory (OVRO), Atacama Large Millimetric Array (ALMA), and the infrared /textit{Spitzer} observatories, are powerful facilities to study massive star formation regions and related objects such as ultra--compact (UC) /hii regions, molecular clumps, and cores. We used these telescopes to study the /uchiir G43.89--0.78. The morphological study at arcminute scales using NVSS and /textit{Spitzer} data shows that this region is similar to those observed in the /textit{ bubble--like} structures revealed by /textit{Spitzer} observations. With this result, and including a physical characterization based on 3.6 cm data, we suggest G43.89--0.78 be classified as an /uchiir with Extended Emission because it meets the operational definition given in this paper comparing radio continuum data at 3.6 and 20~cm. For the ultra-compact component, we use VLA data to obtain physical parameters at 3.6~cm confirming this region as an /uchii region. Using ALMA observations, we detect the presence of a dense ($2.6/times10^7$ cm$^{-3}$) and small ($/sim$ 2.0/arcsec; 0.08 pc) molecular clump with a mass of 220 M$_{/odot}$ and average kinetic temperature of 21~K, located near to the /uchii region. In this clump, catalogued as G43.890--0.784, water masers also exist, possibly tracing a bipolar outflow. We discover in this vicinity two additional clumps which we label as G43.899--0.786 (T$_d$ = 50 K; M = 11 M$_{/odot}$), and G43.888--0.787 (T$_d$ = 50 K; M = 15 M$_{/odot}$).
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2020-07-20
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10.1093/mnras/staa2149
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arxiv
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23f43b83845c7318abd062adbdb145c1cb30c98e
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https://doi.org/10.1093/mnras/staa2149
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Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment
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covid:23f43b83845c7318abd062adbdb145c1cb30c98e#body_text
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