Volume 578, June 2015
|Number of page(s)||19|
|Section||Interstellar and circumstellar matter|
|Published online||01 June 2015|
High spectral and spatial resolution observations of the PDR emission in the NGC 2023 reflection nebula with SOFIA and APEX⋆,⋆⋆,⋆⋆⋆,⋆⋆⋆⋆,†
SOFIA-USRA, NASA Ames Research Center, MS 232-12, Building N232, Rm. 146,
PO Box 1,
2 Tata Institute of Fundamental Research, Homi Bhabha Road, 400005 Mumbai, India
3 Max Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
4 I. Physikalisches Institut der Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany
Received: 12 February 2015
Accepted: 12 April 2015
We have mapped the NGC 2023 reflection nebula in [C ii] and CO(11−10) with the heterodyne receiver GREAT on SOFIA and obtained slightly smaller maps in 13CO(3−2), CO(3−2), CO(4−3), CO(6−5), and CO(7−6) with APEX in Chile. We use these data to probe the morphology, kinematics, and physical conditions of the C ii region, which is ionized by FUV radiation from the B2 star HD 37903. The [C ii] emission traces an ellipsoidal shell-like region at a position angle of ~−50°, and is surrounded by a hot molecular shell. In the southeast, where the C ii region expands into a dense, clumpy molecular cloud ridge, we see narrow and strong line emission from high-J CO lines, which comes from a thin, hot molecular shell surrounding the [C ii] emission. The [C ii] lines are broader and show photo evaporating gas flowing into the C ii region. Based on the strength of the [13C ii] F = 2−1 line, the [C ii] line appears to be somewhat optically thick over most of the nebula with an optical depth of a few. We model the physical conditions of the surrounding molecular cloud and the PDR emission using both RADEX and simple PDR models. The temperature of the CO emitting PDR shell is ~90−120 K, with densities of 105−106 cm-3, as deduced from RADEX modeling. Our PDR modeling indicates that the PDR layer where [C ii] emission dominates has somewhat lower densities, 104 to a few times 105 cm-3.
Key words: ISM: clouds / submillimeter: ISM / ISM: lines and bands / ISM: individual objects: NGC 2023 / ISM: molecules / photon-dominated region (PDR)
The NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA) is jointly operated by the Universities Space Research Association, Inc. (USRA), under NASA contract NAS2-97001, and the Deutsches SOFIA Institut (DSI) under DLR contract 50 OK 0901 to the University of Stuttgart.
The Atacama Pathfinder Experiment (APEX) is a collaboration between the Max-Planck-Institut für Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory.
Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
Appendices are available in electronic form at http://www.aanda.org
Data cubes as FITS files are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (184.108.40.206) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/578/A41
© ESO, 2015
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