J/A+A/588/A104            Molecular clouds and star formation      (Gong+, 2016)

Molecular clouds and star formation toward the Galactic plane within 216.25≤l≤218.75 and -0.75≤b≤1.25. Gong Y., Mao R.Q., Fang M., Zhang S.B., Su Y., Yang J., Jiang Z.B., Xu Y., Wang M., Wang Y., Lu D.R., Sun J.X. <Astron. Astrophys. 588, A104 (2016)> =2016A&A...588A.104G 2016A&A...588A.104G (SIMBAD/NED BibCode)
ADC_Keywords: Galactic plane ; Molecular clouds ; YSOs ; Carbon monoxide Keywords: surveys - ISM: clouds - stars: formation - radio lines: ISM - ISM: kinematics and dynamics Abstract: As a part of the Milky Way Imaging Scroll Painting (MWISP) survey, the aim is to study the physical properties of molecular clouds and their associated star formation toward the Galactic plane within 216.25°≤l≤218.75° and -0.75°≤b≤1.25°, which covers the molecular cloud complex S287. Using the 3x3 Superconducting Spectroscopic Array Receiver (SSAR) at the PMO-13.7m telescope, we performed a simultaneous 12CO (1-0), 13CO (1-0), C18O (1-0) mapping toward molecular clouds in a region encompassing 3.75 square degrees. The beam size is 52" for 12CO (1-0) and 55" for 13CO (1-0) and C18O (1-0). Description: We include three FITS files containing the data-cubes (position-position-velocity) of 12CO, 13CO, and C18O emission lines. We used the Galactic coordinates for the spatial dimensions and V_lsr for the spectral dimension. The pixel size is 30" in spatial dimension and the channel width is about 0.17km/s. All the intensities have been converted to a scale of main beam temperatures in units of K. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 53 3 List of fits datacubes fits/* . 3 Individual fits datacubes tabled1.dat 119 163 The infrared photometric magnitudes of identified YSO candidates in the surveyed region -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 F5.1 deg GLON Galactic longitude of center 6- 10 F5.2 deg GLAT Galactic latitude of center 12- 21 F10.6 MHz nu Rest frequency 23- 24 I2 arcsec FWHM Beam size 26- 28 I3 Mbyte size Size of the fits cube 30- 38 A9 --- FileName Name of the fits cube, in subdirectory fits 40- 53 A14 --- Title Title of the fits file -------------------------------------------------------------------------------- Byte-by-byte Description of file: tabled1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- Name Name (JHHMMSS.ss+DDMMSS.s) 21- 27 F7.3 deg GLON Galactic longitude 29- 34 F6.3 deg GLAT Galactic latitude 36- 40 F5.2 mag Jmag ?=- 2MASS J magnitude 42- 45 F4.2 mag e_Jmag ? rms uncertainty on Jmag 47- 51 F5.2 mag Hmag ?=- 2MASS H magnitude 53- 56 F4.2 mag e_Hmag ? rms uncertainty on Hmag 58- 62 F5.2 mag Ksmag ?=- 2MASS Ks magnitude 64- 67 F4.2 mag e_Ksmag ? rms uncertainty on Ksmag 69- 73 F5.2 mag W1mag ?=- WISE W1 magnitude 75- 78 F4.2 mag e_W1mag ? rms uncertainty on W1mag 80- 84 F5.2 mag W2mag ?=- WISE W2 magnitude 86- 89 F4.2 mag e_W2mag ? rms uncertainty on W2mag 91- 95 F5.2 mag W3mag ?=- WISE W3 magnitude 97-100 F4.2 mag e_W3mag ? rms uncertainty on W3mag 102-105 F4.2 mag W4mag ?=- WISE W4 magnitude 107-110 F4.2 mag e_W4mag ? rms uncertainty on W4mag 113-116 F4.1 mag Av ? Visual Extinxtion 118-119 A2 --- Class [I II] YSO class -------------------------------------------------------------------------------- Acknowledgements: Yan Gong, ygong(at)pmo.ac.cn
(End) Yan Gong [Purple Mountain Obs.], Patricia Vannier [CDS] 26-Feb-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