About: Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment

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About: Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment Goto Sponge NotDistinct Permalink

An Entity of Type : schema:ScholarlyArticle, within Data Space : wasabi.inria.fr associated with source document(s)

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type	Academic Article research paper schema:ScholarlyArticle
isDefinedBy	Covid-on-the-Web dataset
has 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 Nigoche-Netro, Alberto Porras, Alicia Rodríguez-Rico, Carlos Trinidad, Miguel
Source	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$_{/odot}$).
has issue date	2020-07-20(xsd:dateTime)
bibo:doi	10.1093/mnras/staa2149
has license	arxiv
sha1sum (hex)	23f43b83845c7318abd062adbdb145c1cb30c98e
schema:url	https://doi.org/10.1093/mnras/staa2149
resource representing a document's title	Ultracompact HII regions with extended emission: The case of G43.89-0.78 and its molecular environment
resource representing a document's body	covid:23f43b83845c7318abd062adbdb145c1cb30c98e#body_text
is schema:about of	named entity 'mass' named entity 'objects' named entity 'infrared' named entity 'Spitzer' named entity 'For' named entity '3.6' named entity 'OBSERVED' named entity 'PHYSICAL' named entity 'RELATED' named entity 'confirming' named entity 'based' named entity 'telescopes' named entity 'molecular' named entity 'bipolar outflow' named entity 'water masers' named entity 'physical' named entity 'NVSS' named entity 'observatories' named entity '2.0' named entity 'star formation regions' named entity 'NVSS' named entity 'Spitzer' named entity 'ALMA' named entity 'Ultracompact' named entity 'study' named entity 'VLA' named entity '0.1' named entity 'water masers' named entity 'G43' named entity 'water maser' named entity 'LAMDA' named entity 'ionized' named entity 'molecular species' named entity 'H II' named entity 'G43' named entity 'ASIAA' named entity 'G43' named entity 'water masers' named entity 'G43' named entity 'Milky Way' named entity 'velocity' named entity 'kpc' named entity 'high-mass' named entity 'HII region' named entity 'G43' named entity 'G43' named entity 'kpc' named entity 'calibrator' named entity 'calibrator' named entity 'infrared' named entity 'arcmin' named entity 'Monte Carlo' named entity 'spatial resolution' named entity 'NH 3' named entity 'masers' named entity 'IRAC' named entity 'H II' named entity 'G43' named entity 'IRAC' named entity 'Trinidad' named entity 'NH 3' named entity 'GHz' named entity 'H II' named entity 'VLA' named entity 'molecular emission' named entity '0.01' named entity 'field of view' named entity 'ionized gas' named entity 'water masers' named entity 'line emission' named entity 'VLA' named entity 'Onsala' named entity 'angular resolution' named entity 'VLA' named entity 'spectral line' named entity 'kpc' named entity 'ionized gas'

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