Abstract By combining new NRAO 12m data with previously published BIMA data, we have obtained very high signal-to-noise maps of HCO + in the Orion B core, which contain information on both the large- and small-scale emission and put new constraints on the gas’ physical conditions.
Peter J Barnes, Yoshinori Yonekura, Y. Fukui, Andrew T. Miller, M. Mühlegger, Lawrence C. Agars, Yosuke Miyamoto, N. Furukawa, George Papadopoulos, Scott L. Jones, Audra K. Hernandez, Stefan O’Dougherty, Jonathan C. Tan
Discussion(0)
No comments yet. Be the first to comment.