SIMBAD references

2018ApJS..236...25K - Astrophys. J., Suppl. Ser., 236, 25-25 (2018/June-0)

The CARMA-NRO Orion Survey.

KONG S., ARCE H.G., FEDDERSEN J.R., CARPENTER J.M., NAKAMURA F., SHIMAJIRI Y., ISELLA A., OSSENKOPF-OKADA V., SARGENT A.I., SANCHEZ-MONGE A., SURI S.T., KAUFFMANN J., PILLAI T., PINEDA J.E., KODA J., BALLY J., LIS D.C., PADOAN P., KLESSEN R., MAIRS S., GOODMAN A., GOLDSMITH P., McGEHEE P., SCHILKE P., TEUBEN P.J., MAUREIRA M.J., HARA C., GINSBURG A., BURKHART B., SMITH R.J., SCHMIEDEKE A., PINEDA J.L., ISHII S., SASAKI K., KAWABE R., URASAWA Y., OYAMADA S. and TANABE Y.

Abstract (from CDS):

We present the first results from a new, high-resolution 12CO(1-0), 13CO(1-0), and C18O(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 Δ-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 Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): ISM: clouds - ISM: jets and outflows - ISM: kinematics and dynamics - ISM: structure - photon-dominated region PDR - stars: formation

Status in Simbad:  waiting for electronic table

Simbad objects: 23

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2019.12.15-04:30:40

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