Geco - Galactic Science With Ccat-P

The CCAT-p telescope will be a 6m telescope built on Cerro Chajnantor, at an altitude of 5600 m. While a significant portion of the CCAT-p science is dedicated to Galaxy formation or Cosmology, there is also important Galactic Science the instrument can do. In this talk, I will summarize the science we envision to perform mostly with the heterodyne CHAI array: a survey of the Galactic Plane and the Magellanic Clouds in atomic carbon, searching for turbulence dissipation structures in Gould belt clouds, and searching for protostellar variability.

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PID https://www.doi.org/10.5281/zenodo.1159066
PID https://www.doi.org/10.5281/zenodo.1159067
URL http://dx.doi.org/10.5281/zenodo.1159067
URL https://zenodo.org/record/1159067
URL http://dx.doi.org/10.5281/zenodo.1159066
URL https://figshare.com/articles/GEco_-_Galactic_Science_with_CCAT-p/6913367
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Access Right Open Access
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Author Schilke, Peter
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Collected From Datacite; figshare; FigShare
Hosted By Zenodo; figshare; FigShare
Publication Date 2018-01-25
Publisher Zenodo
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Language UNKNOWN
Resource Type Other literature type; Conference object
keyword arxiv.Astrophysics::Instrumentation and Methods for Astrophysics
keyword arxiv.Astrophysics::Earth and Planetary Astrophysics
keyword arxiv.Astrophysics::Cosmology and Extragalactic Astrophysics
keyword arxiv.Astrophysics::High Energy Astrophysical Phenomena
keyword arxiv.Astrophysics::Galaxy Astrophysics
system:type publication
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Source https://science-innovation-policy.openaire.eu/search/publication?articleId=dedup_wf_001::e9e6b3078bc71ff016252605f6917ded
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Last Updated 22 December 2020, 22:20 (CET)
Created 22 December 2020, 22:20 (CET)