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COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey

  • Authors: Thomas J. Rennie, Stuart E. Harper, Clive Dickinson, Liju Philip, Kieran A. Cleary, Richard J. Bond, Jowita Borowska, Patrick C. Breysse, Morgan Catha, Roke Cepeda-Arroita, Dongwoo T. Chung, Sarah E. Church, Delaney A. Dunne, Hans Kristian Eriksen, Marie Kristine Foss, Todd Gaier, Joshua Ott Gundersen, Andrew I. Harris, Brandon Hensley, Richard Hobbs, Håvard T. Ihle, James W. Lamb, Charles R. Lawrence, Jonas G. S. Lunde, Roberta Paladini, Timothy J. Pearson, Maren Rasmussen, Anthony C. S. Readhead, Nils-Ole Stutzer, Duncan J. Watts, Ingunn Kathrine Wehus, David P. Woody

Thomas J. Rennie et al 2022 The Astrophysical Journal 933 .

  • Provider: AAS Journals

Caption: Figure 10.

Plot of emissivities (calculated using the source sizes in Table 3) of all highlighted sources on the Galactic plane at 30 GHz across the different regions. The colored solid lines represent spinning dust models for a range of typical interstellar environments: cold neutral medium (CNM), dark clouds (DC), molecular clouds (MC), reflection nebulae (RN), WIM, warm neutral medium (WNM), and PDR. Sources categorized as AME or non-AME regions are plotted as white squares or filled circles, respectively. The weighted-average values are shown for the AME (dashed line) and non-AME (dotted line) regions.

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