Kong, Shuo, Arce, Hector G., Feddersen, Jesse R., Carpenter, John M., Nakamura, Fumitaka, Shimajiri, Yoshito, Isella, Andrea, Ossenkopf-Okada, Volker ORCID: 0000-0002-8351-3877, Sargent, Anneila I., Sanchez-Monge, Alvaro, Suri, Suemeyye T., Kauffmann, Jens ORCID: 0000-0002-5094-6393, Pillai, Thushara, Pineda, Jaime E., Koda, Jin, Bally, John, Lis, Dariusz C., Padoan, Paolo ORCID: 0000-0002-5055-5800, Klessen, Ralf, Mairs, Steve ORCID: 0000-0002-6956-0730, Goodman, Alyssa, Goldsmith, Paul, McGehee, Peregrine ORCID: 0000-0003-0948-6716, Schilke, Peter ORCID: 0000-0003-2141-5689, Teuben, Peter J., Jose Maureira, Maria, Hara, Chihomi, Ginsburg, Adam, Burkhart, Blakesley, Smith, Rowan J., Schmiedeke, Anika, Pineda, Jorge L., Ishii, Shun ORCID: 0000-0001-8337-4961, Sasaki, Kazushige, Kawabe, Ryohei, Urasawa, Yumiko, Oyamada, Shuri and Tanabe, Yoshihiro (2018). The CARMA-NRO Orion Survey. Astrophys. J. Suppl. Ser., 236 (2). BRISTOL: IOP PUBLISHING LTD. ISSN 1538-4365

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Abstract

We present the first results from a new, high-resolution (CO)-C-12(1-0), (CO)-C-13(1-0), and (CO)-O-18(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 45 m 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.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Kong, ShuoUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Arce, Hector G.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Feddersen, Jesse R.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Carpenter, John M.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Nakamura, FumitakaUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Shimajiri, YoshitoUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Isella, AndreaUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Ossenkopf-Okada, VolkerUNSPECIFIEDorcid.org/0000-0002-8351-3877UNSPECIFIED
Sargent, Anneila I.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Sanchez-Monge, AlvaroUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Suri, Suemeyye T.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Kauffmann, JensUNSPECIFIEDorcid.org/0000-0002-5094-6393UNSPECIFIED
Pillai, ThusharaUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Pineda, Jaime E.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Koda, JinUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Bally, JohnUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Lis, Dariusz C.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Padoan, PaoloUNSPECIFIEDorcid.org/0000-0002-5055-5800UNSPECIFIED
Klessen, RalfUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Mairs, SteveUNSPECIFIEDorcid.org/0000-0002-6956-0730UNSPECIFIED
Goodman, AlyssaUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Goldsmith, PaulUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
McGehee, PeregrineUNSPECIFIEDorcid.org/0000-0003-0948-6716UNSPECIFIED
Schilke, PeterUNSPECIFIEDorcid.org/0000-0003-2141-5689UNSPECIFIED
Teuben, Peter J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Jose Maureira, MariaUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Hara, ChihomiUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Ginsburg, AdamUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Burkhart, BlakesleyUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Smith, Rowan J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Schmiedeke, AnikaUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Pineda, Jorge L.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Ishii, ShunUNSPECIFIEDorcid.org/0000-0001-8337-4961UNSPECIFIED
Sasaki, KazushigeUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Kawabe, RyoheiUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Urasawa, YumikoUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Oyamada, ShuriUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Tanabe, YoshihiroUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-185580
DOI: 10.3847/1538-4365/aabafc
Journal or Publication Title: Astrophys. J. Suppl. Ser.
Volume: 236
Number: 2
Date: 2018
Publisher: IOP PUBLISHING LTD
Place of Publication: BRISTOL
ISSN: 1538-4365
Language: English
Faculty: Faculty of Mathematics and Natural Sciences
Divisions: Faculty of Mathematics and Natural Sciences > Department of Physics > Institute of Physics I
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
SUBMILLIMETER-WAVE OBSERVATIONS; INTEGRAL-SHAPED FILAMENT; TAURUS MOLECULAR CLOUD; STAR-FORMING FILAMENTS; H II REGION; MAGNETIC-FIELDS; DELTA-VARIANCE; MILKY-WAY; CO SURVEY; TURBULENCEMultiple languages
Astronomy & AstrophysicsMultiple languages
Refereed: Yes
URI: http://kups.ub.uni-koeln.de/id/eprint/18558

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