J/MNRAS/452/3969    ATCA Survey of Sagittarius B2 at 7mm         (Corby+, 2015)

An ATCA survey of Sagittarius B2 at 7 mm: chemical complexity meets broad-band interferometry. Corby J.F., Jones P.A., Cunningham M.R., Remijan A.J., Menten K.M., Belloche A., Schwab F., Walsh A., Balnozan E., Bronfman L., Lo N. <Mon. Not. R. Astron. Soc. 452, 3969 (2015)> =2015MNRAS.452.3969C 2015MNRAS.452.3969C
ADC_Keywords: Molecular clouds ; Radio lines ; Radio continuum ; Spectroscopy ; H II regions ; Nebulae Keywords: astrochemistry - line: identification - H II regions - ISM: molecules - photodissociation region (PDR) - radio lines: ISM Abstract: We present a 30-50GHz survey of Sagittarius B2(N) conducted with the Australia Telescope Compact Array (ATCA) with 5 - 10 arcsec resolution. We analyze the spectra towards three HII regions that have foreground molecular gas in Sgr B2. Towards the most line-dense region, we detect >500 spectral line components, >90% of which are assigned to H and He recombination lines and 53 firmly identified molecular species (not including isotopologues). The data reveal extremely subthermally excited molecular gas in Sgr B2 absorbing against the continuum background, as well as molecular line emission from two hot cores in Sgr B2(N). They also also contain line-of-sight absorption by ∼15 molecules observed in translucent gas in the Galactic Center, bar, and intervening spiral arm clouds, revealing the complex chemistry and clumpy structure of this gas. Formamide (NH2CHO) is detected for the first time in a translucent cloud. Description: The FITS files include 12 baseline-subtracted data cubes that are not corrected for the primary beam. The data cover the full frequency range from 29.8-50.2GHz with 1MHz channels and three continuum images. The data were taken towards a single pointing position towards Sgr B2(N). The continuum images are all generated from a 7.5GHz bandwidth, and the three images are centered on 33.4GHz, 40.2GHz, and 46.5GHz. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 17 47 20.4 -28 22 12 Sgr B2 = NAME SGR B2 ------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 234 15 List of fits images and data cubes fits/* . 15 Individual fits data cubes -------------------------------------------------------------------------------- See also: J/ApJS/117/427 : Sgr B2 spectral survey (Nummelin+, 1998) J/ApJS/158/188 : Detection of glycolaldehyde toward Sgr B2 (Widicus+, 2005) J/A+A/559/A47 : Sgr B2(N) and Sgr B2(M) IRAM 30m line survey (Belloche+, 2013) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 "datime" ObsDate Observation date 21- 29 F9.5 deg RAdeg Right Ascension of center (J2000) 30- 38 F9.5 deg DEdeg Declination of center (J2000) 39- 41 F3.1 arcsec/pix Scale [1/2] Scale of the image 43- 45 I3 --- Nx [160/256] Number of pixels along X-axis 47- 49 I3 --- Ny [160/256] Number of pixels along Y-axis 51- 54 I4 --- Nz [1/1948] Number of slides or channels 56- 60 I5 MHz nu.min [29776/48276] Lower value of Frequency 62- 66 I5 MHz nu.max [31724/50224] Upper value of Frequency 68- 70 F3.1 MHz dnu [1.0] Frequency resolution [MHz] 72- 78 F7.3 Mbyte size [0.121/488] Size of FITS file 80-110 A31 --- FileName Name of FITS file, in "fits" subdirectory 112-234 A123 --- Title Title of the file -------------------------------------------------------------------------------- Acknowledgements: Joanna Corby, jfc2113(at)gmail.com Paul Jones, paulcojones(at)gmail.com National Radio Astronomy Observatory; Australia Telescope National Facility of the CSIRO, Australia
(End) Patricia Vannier [CDS] 29-May-2015
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