Large Scale CO and [CI] emission in the rho Ophiuchi Molecular Cloud
arXiv:astro-ph/0408518 · doi:10.1086/426096
Abstract
We present a comprehensive study of the rho Ophiuchi molecular cloud that addresses aspects of the physical structure and condition of the molecular cloud and its photodissociation region (PDR) by combining far-infrared and submillimeter-wave observations with a wide range of angular scale and resolution. We present 40'x40' maps in CO(4-3) and [CI](3P1-3P0) line emission from the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO), and pointed observations in the CO(7-6) and [CI](3P2-3P1) lines. Within, smaller spectral line maps of the cloud in CO, CS, HCO+ and their rare isotopomers are made at the Heinrich Hertz Submillimeter Telescope Observatory (HHT) in Arizona. Comparison with far-infrared and submillimeter continuum emission, and near-infrared H2 emission allows clearer determination of the physical and chemical structure of the rho Oph photodissociation region (PDR). The excitation conditions needed to produce the observed HCO+ and [OI] emission directly imply inhomogeneous structure. Strong chemical gradients are observed in HCO+ and CS; the former is ascribed to a local enhancement in the H2 ionization rate, the latter is principally due to shocks. The distribution of [CI] is very similar to C18O, and generally consistent with illumination from the 'far' side of the cloud. A notable exception is found at the the western edge of the cloud, where UV photons create a PDR viewed `edge-on'. The abundance of atomic carbon is accurately modeled using a radiation field that decreases with increasing projected distance from the exciting star HD147889. In contrast to conclusions of other studies, we find that no non-equilibrium chemistry is needed to enhance the atomic carbon abundance.
arXiv comment17 pages, 21 figures. To be published in the Astrophysical Journal. High resolution color version (PS, PDF formats) available at http://loke.as.arizona.edu/~ckulesa/research/publications/rhooph/
References in corpus (8)
- The Milky Way in Molecular Clouds: A New Complete CO Survey
- Structure of Stationary Photodissociation Fronts
- Far Infrared and Submillimeter Emission from Galactic and Extragalactic Photo-Dissociation Regions
- Water Abundance in Molecular Cloud Cores
- The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO)
- Chandra and ASCA Observations of the X-ray-brightest T-Tauri Stars in the Rho Ophiuchi Cloud
- Submillimeter Continuum Emission in the Rho Ophiuchus Molecular Cloud: Filaments, Arcs, and an Unidentified Infrared Object
- Chandra Observations of a Young Embedded Magnetic B Star in the rho Ophiuchus Cloud
Cited by in corpus (24)
- Molecular Hydrogen in the FUSE Translucent Lines of Sight: The Full Sample
- Planck early results. XX. New light on anomalous microwave emission from spinning dust grains
- Molecular oxygen in the rho Ophiuchi cloud
- The Extended Environment of M17: A Star Formation History
- Multi-line detection of O2 toward rho Oph A
- Radio Recombination Lines in Galactic HII Regions
- The Role of Galactic Winds on Molecular Gas Emission from Galaxy Mergers
- Star Forming Dense Cloud Cores in the TeV γ-ray SNR RX J1713.7-3946
- An Alternative Accurate Tracer of Molecular Clouds: The "-Factor"
- Astronomy in Antarctica
- The JCMT Legacy Survey of the Gould Belt: a molecular line study of the Ophiuchus molecular cloud
- Spitzer and HHT observations of starless cores: masses and environments
- Star formation in W3 - AFGL333: Young stellar content, properties and roles of external feedback
- On the nature of outflows in intermediate-mass protostars: a case study of IRAS 20050+2720
- A CO Line and Infrared Continuum Study of the Active Star-Forming Complex W51
- Who Is Eating the Outflow?: High-Angular Resolution Study of an Intermediate-Mass Protostar in L1206
- Astrochemical Correlations in Molecular Clouds
- Triggered Star Formation in a Double Shell near W51A
- Spitzer observations of a 24 micron shadow: Bok Globule CB190
- A CO (J=3-2) Outflow Survey of the Elias 29 Region
- The Astrochemical Impact of Cosmic Rays in Protoclusters II: CI-to-H and CO-to-H Conversion Factors
- Oxygen in dense interstellar gas - the oxygen abundance of the star forming core rho Oph A
- Molecular gas properties of Q1700-MD94: a massive, main-sequence galaxy at
- Deep kiloparsec view of the molecular gas in a massive star-forming galaxy at cosmic noon