J/A+A/655/L2           OGHReS 12CO(2-1) data cubes              (Colombo+, 2021)

OGHReS: large-scale filaments in the outer Galaxy. Colombo D., Koenig C., Urquhart J.S., Wyrowski F., Mattern M., Menten K.M., Lee M.-Y., Brand J., Wienen M., Mazumdar P., Schuller F., Leurini S. <Astron. Astrophys. 655, L2 (2021)> =2021A&A...655L...2C 2021A&A...655L...2C (SIMBAD/NED BibCode)
ADC_Keywords: Interstellar medium ; Carbon monoxide Keywords: ISM: molecules - ISM: clouds - evolution - ISM: structure - local interstellar matter - galaxies: ISM Abstract: Filaments are a ubiquitous morphological feature of the molecular interstellar medium and are identified as sites of star formation. In recent years, more than 100 large-scale filaments (with length >10pc) have been observed in the inner Milky Way. As they appear linked to Galactic dynamics, studying those structures represents an opportunity to link kpc-scale phenomena to the physics of star formation, which operates on much smaller scales. In this letter, we use newly acquired Outer Galaxy High Resolution Survey (OGHReS) 12CO(2-1) data to demonstrate that a significant number of large-scale filaments are present in the outer Galaxy as well. The 37 filaments identified appear tightly associated to inter-arm regions. In addition, their masses and linear masses are, on average, one order of magnitude lower than similar-sized molecular filaments located in the inner Galaxy, showing that Milky Way dynamics is able to create very elongated features in spite of the lower gas supply in the Galactic outskirts. Description: Datacubes used in the paper. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 112 37 List of fits datacubes fits/* . 37 Individual fits datacubes -------------------------------------------------------------------------------- See also: J/A+A/619/A166 : SEDIGISM, kinematics of ATLASGAL filaments (Mattern+, 2018) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- --- [G] 2- 10 F9.5 deg GLON Galacitc longitude 11- 19 F9.5 deg GLAT Galactic latitude 21- 23 I3 --- Nx Number of pixels along X-axis 25- 27 I3 --- Ny Number of pixels along Y-axis 29- 30 I2 --- Nz Number of pixels along Z-axis 32- 36 I5 m/s bVRAD Lower value of VRAD interval 38- 42 I5 m/s BVRAD Upper value of VRAD interval 44- 46 I3 m/s dVRAD VRAD resolution 48- 52 I5 Kibyte size Size of FITS file 54- 86 A33 --- FileName Name of FITS file, in subdirectory fits 88-112 A25 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Dario Colombo, dcolombo(at)mpifr-bonn.mpg.de References: Taylor & Cordes, 1993ApJ...411..674T 1993ApJ...411..674T Rosolowsky et al., 2008ApJ...679.1338R 2008ApJ...679.1338R Reid et al., 2016ApJ...823...77R 2016ApJ...823...77R Zucker et al., 2018ApJ...864..153Z 2018ApJ...864..153Z Amari & Aly, 2010A&A...522A..52A 2010A&A...522A..52A
(End) Patricia Vannier [CDS] 29-Oct-2021
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