Characterizing the transition from diffuse atomic to dense molecular clouds in the Magellanic clouds with [CII], [CI], and CO

https://doi.org/10.26131/IRSA516
https://www.ipac.caltech.edu/doi/10.26131/IRSA516

10.26131/IRSA516

IPAC

Pineda, Jorge L.; Langer, William D.; Goldsmith, Paul F.; Horiuchi, Shinji; Kuiper, Thomas B. H.; Muller, Erik; Hughes, Annie; Ott, Jürgen; Requena-Torres, Miguel A.; Velusamy, Thangasamy; Wong, Tony

Characterizing the transition from diffuse atomic to dense molecular clouds in the Magellanic clouds with [CII], [CI], and CO

Herschel data from the "Characterizing the transition from diffuse atomic to dense molecular clouds in the Magellanic clouds with [CII], [CI], and CO" (MAGCLOUDSCPLUS) Open Time Key Program (KPOT_jpineda_1) are available here using spatial and visualization tools. MAGCLOUDSCPLUS surveyed 54 lines of sight toward the Large and Small Magellanic Clouds in the [C II] 158 micron, [C I] 609 micron, [C I] 370 micron, and 12CO J = 7 → 6 lines using Herschel's HIFI instrument.

This dataset or service is made available by the Infrared Science Archive (IRSA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Dataset

https://irsa.ipac.caltech.edu/data/Herschel/MAGCLOUDSCPLUS

2018-12-14