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J/A+A/474/911 1.3mm and CO(1-0) maps of IRAS 20343+4129 (Palau+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
maps.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/474/911
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drwxr-xr-x 16 cats archive 277 Feb 7 2018 [Up]
drwxr-xr-x 3 cats archive 224 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 469 Dec 19 2022 .message
-r--r--r-- 1 cats archive 2868 Dec 30 2007 ReadMe
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-r--r--r-- 1 cats archive 149 Dec 30 2007 maps.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/A+A/474/911 1.3mm and CO(2-1) maps of IRAS 20343+4129 (Palau+, 2007)
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Unveiling the nature and interaction of the intermediate/high-mass YSOs
in IRAS 20343+4129.
Palau A., Estalella R., Ho P.T.P., Beuther H., Beltran M. T.
<Astron. Astrophys. 474, 911 (2007)>
=2007A&A...474..911P (SIMBAD/NED BibCode)
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ADC_Keywords: Infrared sources ; Millimetric/submm sources
Keywords: stars: formation - ISM: individual: IRAS 20343+4129 -
ISM: dust, extinction - ISM: clouds
Abstract:
IRAS 20343+4129 was suggested to harbor one of the most massive and
embedded stars in the Cygnus OB2 association, IRS 1, which seemed to
be associated with a north-south molecular outflow. However, the dust
emission peaks do not coincide with the position of IRS 1, but lie on
either side of another massive Young Stellar Object (YSO), IRS 3,
which is associated with centimeter emission.
The goal of this work is to elucidate the nature of IRS 1 and IRS 3,
and study their interactions with the surrounding medium.
Description:
One of the first observations with the Submillimeter Array with six
antennas on the array. We observed the 1.3mm continuum and CO(2-1)
line toward one high-mass protostellar object candidate.
Objects:
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RA (2000) DE Designation(s)
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20 36 07.1 +41 40 01 IRAS 20343+4129 = IRAS 20343+4129
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