/ftp/cats/J_A+A/510/A5



==========================================================================
J/A+A/510/A5        CO(2-1) maps of IRAS 00117+6412          (Palau+, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
	maps.dat
==========================================================================
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/510/A5
==========================================================================

drwxr-xr-x 20 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 3 cats archive 4096 Dec 15 2013 [TAR file] -rw-r--r-- 1 cats archive 458 Apr 9 2010 .message -r--r--r-- 1 cats archive 3796 Apr 9 2010 ReadMe -rw-r--r-- 1 cats archive 240 Apr 9 2010 +footg5.gif -rw-r--r-- 1 cats archive 2070 Apr 9 2010 +footg8.gif drwxr-xr-x 2 cats archive 4096 Nov 20 2009 fig -r--r--r-- 1 cats archive 960 Apr 9 2010 maps.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/510/A5 CO(2-1) maps of IRAS 00117+6412 (Palau+, 2010) ================================================================================ Three intermediate-mass young stellar objects with different properties emerging from the same natal cloud in IRAS 00117+6412. Palau A., Sanchez-Monge A., Busquet G., Estalella R., Zhang Q., Ho P.T.P., Beltran M.T., Beuther H. <Astron. Astrophys. 510, A5 (2010)> =2010A&A...510A...5P ================================================================================ ADC_Keywords: Infrared sources ; YSOs ; Radio sources Keywords: stars: formation - dust, extinction - HII regions - ISM: individual objects: IRAS 00117+6412 - radio continuum: ISM Abstract: Our main aim is to study the influence of the initial conditions of a cloud in the intermediate/high-mass star formation process. We observed with the VLA, PdBI, and SMA the centimeter and millimeter continuum, N_2_H^+^ (1-0), and CO (2-1) emission associated with a dusty cloud harboring a nascent cluster with intermediate-mass protostars. Description: Interferometric observations of centimeter and millimeter continuum, dense gas, and CO(2-1) emission of an embedded cluster with at least three very young intermediate-mass protostars with different properties. The goal is to study the role of initial conditions in the intermediate/high-mass star formation process. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 00 14 26.6 +64 28 30 IRAS 00117+6412 = LEDA 2796303 ----------------------------------------------------------

© Unistra/CNRS

Contact