GBT Multiwavelength Survey of the Galactic Center Region
arXiv:0801.4294 · doi:10.1086/533587
Abstract
We describe the results of a radio continuum survey of the central 4x1deg with the 100 m Green Bank Telescope (GBT) at wavelengths of 3.5, 6, 20, and 90 cm. The 3.5 and 6 cm surveys are the most sensitive and highest resolution single dish surveys made of the central degrees of our Galaxy. We present catalogs of compact and extended sources in the central four degrees of our Galaxy, including detailed spectral index studies of all sources. The analysis covers star-forming regions such as Sgr B and Sgr C where we find evidence of a mixture of thermal and nonthermal emission. The analysis quantifies the relative contribution of thermal and nonthermal processes to the radio continuum flux density toward the GC region. In the central 4x1deg of the GC, the thermal and nonthermal flux fractions for all compact and diffuse sources are 28%/72% at 3.5 cm and 19%/81% at 6 cm. The total flux densities from these sources are 783+-52 Jy and 1063+-93 Jy at 3.5 and 6 cm, respectively, excluding the contribution of Galactic synchrotron emission.
arXiv commentAccepted to ApJS. 40 pages, 46 figures, 8 tables (emulate apj style)
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- Fourier Plane Image Combination by Feathering
- The QUaD Galactic Plane Survey II: A Compact Source Catalog
- 74 MHz Nonthermal Emission from Molecular Clouds: Evidence for a Cosmic Ray Dominated Region at the Galactic Center
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- A Constraint on the Organization of the Galactic Center Magnetic Field Using Faraday Rotation
- The physical and chemical structure of Sagittarius B2 -- VI. UCHII regions in Sgr B2
- X-ray Observation of a Magnetized Hot Gas Outflow in the Galactic Center Region
- Cosmic-Ray Models of the Ridge-Like Excess of Gamma Rays in the Galactic Center
- A 6.7 GHz methanol maser survey of the central molecular zone
- Multi-epoch searches for relativistic binary pulsars and fast transients in the Galactic Centre
- Towards a three-dimensional distribution of the molecular clouds in the Galactic Centre
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- Stochastic Acceleration of Cosmic Rays in the Central Molecular Zone of the Galaxy
- The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
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- SOFIA-upGREAT imaging spectroscopy of the [C II] 158um fine structure line of the Sgr B region in the Galactic center
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- The connecting molecular ridge in the Galactic center
- Imprints of Molecular Clouds in Radio Continuum Images
- Suzaku Discovery of Twin Thermal Plasma from the Tornado Nebula
- Electroweak Dark Matter
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- 4-8 GHz Fourier-domain Searches for Galactic Center Pulsars