Image Details

Choose export citation format:

Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey

  • Authors: Ken'ichi Tatematsu, Gwanjeong Kim, Tie Liu, Neal J. Evans II, Hee-Weon Yi, Jeong-Eun Lee, Yuefang Wu, Naomi Hirano, Sheng-Yuan Liu, Somnath Dutta, Dipen Sahu, Patricio Sanhueza, Kee-Tae Kim, Mika Juvela, L. Viktor Tóth, Orsolya Fehér, Jinhua He, J. X. Ge, Siyi Feng, Minho Choi, Miju Kang, Mark A. Thompson, Gary A. Fuller, Di Li, Isabelle Ristorcelli, Ke Wang, James Di Francesco, David Eden, Satoshi Ohashi, Ryo Kandori, Charlotte Vastel, Tomoya Hirota, Takeshi Sakai, Xing Lu, Quang Nguyên Lu'o'ng, Hiroko Shinnaga, and Jungha Kim

2021 The Astrophysical Journal Supplement Series 256 25.

  • Provider: AAS Journals

Caption: Figure 16.

Close-up maps sorted in order of evolutionary stages using Tbol for representative star-forming cores. Each map represents the integrated-intensity contour map superposed on the 850 μm dust continuum emission map. The orange, green, and blue contours represent the N2H+, CCS-H, and CCS-L integrated-intensity contour maps, respectively. The innermost to outermost contour levels correspond to 95%, 80%, 65%, 50%, 35%, 20%, 5%, and 3σ, respectively. The σ and peak values of integrated intensity are listed in Table A3. The cross and stars represent a SCUBA-2 core and a protostar, respectively. The error for Tbol is listed in Table A2 in the appendix.

Other Images in This Article

Show More

Copyright and Terms & Conditions