Access to Astronomical Catalogues

← Click to display the menu
J/A+A/503/859   IRDC 19175-4 and IRDC 19175-5 turbulence maps   (Beuther+, 2009)

Multiple low-turbulence starless cores associated with intermediate- to high-mass star formation. Beuther H., Henning T. <Astron. Astrophys. 503, 859 (2009)> =2009A&A...503..859B
ADC_Keywords: Molecular clouds ; Millimetric/submm sources ; Radio lines Keywords: stars: formation - stars: individual: IRDC 19175-4, IRDC 19175-5 - techniques: interferometric - line: formation - line: profiles - turbulence Abstract: The aims is to characterizing the gas and dust properties prior to and in the neighborhood of active intermediate- to high-mass star formation. Two Infrared Dark Clouds (IRDCs), IRDC 19175-4 and IRDC 19175-5, that are located in the vicinity of the luminous massive star-forming region IRAS 19175+1357, but that remain absorption features up to 70um wavelength, were observed with the Plateau de Bure Interferometer in the 3.23mm dust continuum as well as the N2H+(1-0) and 13CS(2-1) line emission. Objects: -------------------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------------------- 19 19 49.1 +14 02 46 IRAS 19175+1357 = IRAS 19175+1357 19 19 50.6 +14 01 22 IRDC 19175-4 = [BSM2002] 19175+1357 4 19 19 49.6 +14 01 09 IRDC 19175-5 = [BSM2002] 19175+1357 5 -------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file maps.dat 103 15 Files list fig/* 0 15 Maps in FITS format
Byte-by-byte Description of file: maps.dat
Bytes Format Units Label Explanations
1- 29 A29 --- FileName Name of the FITS file in subdirectory fig 31-103 A73 --- Title Title of the file
Acknowledgements: Henrik Beuther, beuther(at)mpia-hd.mpg.de
(End) Patricia Vannier [CDS] 14-Jul-2009
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

catalogue service

© UDS/CNRS

Contact