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J/A+A/597/A74       FeSt 1-457 IRAM and PdBI maps            (Juarez+, 2017)

A correlation between chemistry, polarization and dust properties in the Pipe nebula starless core FeSt 1-457. Juarez C., Girart J.M., Frau P., Palau A., Estalella R., Morata O., Alves F.O., Beltran M.T., Padovani, M. <Astron. Astrophys. 597, A74 (2017)> =2017A&A...597A..74J (SIMBAD/NED BibCode)
ADC_Keywords: Molecular clouds ; Radio lines Keywords: stars: formation - ISM: individual objects: FeSt 1-457 nebula - ISM: molecules - radiative transfer Abstract: Pre-stellar cores within molecular clouds provide the very initial conditions in which stars are formed. FeSt 1-457 is a prototypical starless core and the most chemically evolved among those isolated, embedded in the most pristine part of the Pipe nebula, the bowl. We use the IRAM 30m telescope and the PdBI to study the chemical and physical properties of the starless core FeSt 1-457 (Core 109) in the Pipe nebula. We fit the hyperfine structure of the N2H+ (1-0) IRAM 30m data. This allowed us to measure with high precision the velocity field, line widths and opacity and derive the excitation temperature and column density in the core. We used a modified Bonnor-Ebert sphere model adding a temperature gradient towards the center to fit the 1.2mm continuum emission and visual extinction maps. Using this model, we have estimated the abundances of the N2H+ and the rest of molecular lines detected in the 30GHz wide line survey performed at 3mm with IRAM 30m using ARTIST software. Description: IRAM 30m (FTS correlator) and PdBI 3mm observations towards the starless core FeSt 1-457 in the Pipe nebula. Dense core tracer N2H+ (1-0) was observed with a better spectral resolution with the IRAM 30m VESPA correlator (0.06km/s). Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 17 35 45 -25 33.2 FeSt 1-457 = DCld 001.6+03.8 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file list.dat 117 19 List of fits files fits/* 0 19 Indifividual fits files
Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20- 22 I3 --- Nx Number of pixels along X-axis 24- 26 I3 --- Ny Number of pixels along Y-axis 28- 30 I3 --- Nz ? Number of slices for the datacube 32- 34 I3 Kibyte size Size of FITS file 36- 48 A13 --- FileName Name of FITS file, in subdirectory fits 50-117 A68 --- Title Title of the FITS file
Acknowledgements: Carmen Juarez, juarez(at)ice.cat
(End) Carmen Juarez [CSIC-IEEC, Spain], Patricia Vannier [CDS] 31-Oct-2016
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

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