The CARMA-NRO Orion Survey
We present the first results from a new, high resolution, \(^{12}\)CO(1-0), \(^{13}\)CO(1-0), and C\(^{18}\)O(1-0) molecular line survey of the Orion A cloud, hereafter referred to as the CARMA-NRO Orion Survey. CARMA observations have been combined with single-dish data from the Nobeyama 45m telesc...
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| creator | Kong, Shuo Arce, Héctor G Feddersen, Jesse R Carpenter, John M Nakamura, Fumitaka Shimajiri, Yoshito Isella, Andrea Ossenkopf-Okada, Volker Sargent, Anneila I Sánchez-Monge, Álvaro Suri, Sümeyye T Kauffmann, Jens Pillai, Thushara Pineda, Jaime E Koda, Jin Bally, John Lis, Dariusz C Padoan, Paolo Klessen, Ralf Mairs, Steve Goodman, Alyssa Goldsmith, Paul McGehee, Peregrine Schilke, Peter Teuben, Peter J Maureira, María José Hara, Chihomi Ginsburg, Adam Burkhart, Blakesley Smith, Rowan J Schmiedeke, Anika Pineda, Jorge L Ishii, Shun Sasaki, Kazushige Kawabe, Ryohei Urasawa, Yumiko Oyamada, Shuri Tanabe, Yoshihiro |
| description | We present the first results from a new, high resolution, \(^{12}\)CO(1-0), \(^{13}\)CO(1-0), and C\(^{18}\)O(1-0) molecular line survey of the Orion A cloud, hereafter referred to as the CARMA-NRO Orion Survey. CARMA observations have been combined with single-dish data from the Nobeyama 45m telescope to provide extended images at about 0.01 pc resolution, with a dynamic range of approximately 1200 in spatial scale. Here we describe the practical details of the data combination in uv space, including flux scale matching, the conversion of single dish data to visibilities, and joint deconvolution of single dish and interferometric data. A \(\Delta\)-variance analysis indicates that no artifacts are caused by combining data from the two instruments. Initial analysis of the data cubes, including moment maps, average spectra, channel maps, position-velocity diagrams, excitation temperature, column density, and line ratio maps provides evidence of complex and interesting structures such as filaments, bipolar outflows, shells, bubbles, and photo-eroded pillars. The implications for star formation processes are profound and follow-up scientific studies by the CARMA-NRO Orion team are now underway. We plan to make all the data products described here generally accessible; some are already available at https://dataverse.harvard.edu/dataverse/CARMA-NRO-Orion |
| doi_str_mv | 10.48550/arxiv.1803.11522 |
| format | Article |
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CARMA observations have been combined with single-dish data from the Nobeyama 45m telescope to provide extended images at about 0.01 pc resolution, with a dynamic range of approximately 1200 in spatial scale. Here we describe the practical details of the data combination in uv space, including flux scale matching, the conversion of single dish data to visibilities, and joint deconvolution of single dish and interferometric data. A \(\Delta\)-variance analysis indicates that no artifacts are caused by combining data from the two instruments. Initial analysis of the data cubes, including moment maps, average spectra, channel maps, position-velocity diagrams, excitation temperature, column density, and line ratio maps provides evidence of complex and interesting structures such as filaments, bipolar outflows, shells, bubbles, and photo-eroded pillars. The implications for star formation processes are profound and follow-up scientific studies by the CARMA-NRO Orion team are now underway. 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CARMA observations have been combined with single-dish data from the Nobeyama 45m telescope to provide extended images at about 0.01 pc resolution, with a dynamic range of approximately 1200 in spatial scale. Here we describe the practical details of the data combination in uv space, including flux scale matching, the conversion of single dish data to visibilities, and joint deconvolution of single dish and interferometric data. A \(\Delta\)-variance analysis indicates that no artifacts are caused by combining data from the two instruments. Initial analysis of the data cubes, including moment maps, average spectra, channel maps, position-velocity diagrams, excitation temperature, column density, and line ratio maps provides evidence of complex and interesting structures such as filaments, bipolar outflows, shells, bubbles, and photo-eroded pillars. The implications for star formation processes are profound and follow-up scientific studies by the CARMA-NRO Orion team are now underway. We plan to make all the data products described here generally accessible; some are already available at https://dataverse.harvard.edu/dataverse/CARMA-NRO-Orion</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1803.11522</doi><oa>free_for_read</oa></addata></record> |
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| language | eng |
| recordid | cdi_arxiv_primary_1803_11522 |
| source | arXiv.org; Free E- Journals |
| subjects | Cubes Data analysis Filaments Outflow Physics - Astrophysics of Galaxies Pillars Star & galaxy formation Star formation Variance analysis |
| title | The CARMA-NRO Orion Survey |
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