J/A+A/617/A77       Orion Bar Herschel/PACS CO maps            (Parikka+, 2018)

High-J CO emission spatial distribution and excitation in the Orion Bar. Parikka A., Habart E., Bernard-Salas J., Koehler M., Abergel A. <Astron. Astrophys. 617, A77 (2018)> =2018A&A...617A..77P 2018A&A...617A..77P (SIMBAD/NED BibCode)
ADC_Keywords: Molecular clouds; Interstellar medium; Carbon monoxide Keywords: ISM: individual objects: Orion Bar - ISM: lines and bands - photon-dominated region Abstract: With Herschel, we can for the first time observe a wealth of high-J CO lines in the interstellar medium with a high angular resolution. These lines are specifically useful for tracing the warm and dense gas and are therefore very appropriate for a study of strongly irradiated dense photodissocation regions (PDRs). We characterize the morphology of CO J=19-18 emission and study the high-J CO excitation in a highly UV-irradiated prototypical PDR, the Orion Bar. We used fully sampled maps of CO J=19-18 emission with the Photoconductor Array Camera and Spectrometer (PACS) on board the Herschel Space Observatory over an area of ∼110"x110" with an angular resolution of 9". We studied the morphology of this high-J CO line in the Orion Bar and in the region in front and behind the Bar, and compared it with lower-J lines of CO from J=5-4 to J=13-12 and 13CO from J=5-4 to J=11-10 emission observed with the Herschel Spectral and Photometric Imaging Receiver (SPIRE). In addition, we compared the high-J CO to polycyclic aromatic hydrocarbon (PAH) emission and vibrationally excited H2. We used the CO and 13CO observations and the RADEX model to derive the physical conditions in the warm molecular gas layers. Description: We observed the CO J=19-18 line (137um) in the Orion Bar with the Herschel/PACS instrument. The observations were carried out on September 15, 2012, and the total duration was 2687s. A 4x4 raster map was observed for a total area of ∼110"x110" with full Nyquist sampling. Each footprint in the raster map is composed of 5x5 spatial pixels. Objects: ----------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------- 05 35 22.30 -05 24 33.0 Orion Bar = NAME Ori Bar ----------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 121 26 List of fits maps fits/* . 26 Individual fits maps -------------------------------------------------------------------------------- See also: J/ApJ/838/152 : Deep NIR spectrum of the Orion Bar PDR (Kaplan+, 2017) 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- 21 I2 --- Nx Number of pixels along X-axis 23- 24 I2 --- Ny Number of pixels along Y-axis 26- 48 A23 "datime" Obs.date Observation date (YYYY/MM/DDThh:mm:ss.sss) 50- 51 I2 Kibyte size Size of FITS file 53- 84 A32 --- FileName Name of FITS file in subdirectory fits 86-121 A36 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Anna Parikka, parikka(at)ph1.uni-koeln.de
(End) Patricia Vannier [CDS] 19-Sep-2018
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