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The TOP-SCOPE survey of Planck Galactic Cold Clumps: The 200 brightest compact sources of Planck

Published online by Cambridge University Press:  13 January 2020

R. Bögner ,
T. Liu ,
D. J. Eden  and
L. V. Tóth Open the ORCID record for L. V. Tóth [Opens in a new window]
R. Bögner
Affiliation:
Department of Astronomy, Eötvös Loránd University, 1/A Pázmány Péter sétány, 1117 Budapest, Hungary email: [email protected]
T. Liu
Affiliation:
Korea Astronomy and Space Science Institute, 776 Daedeokdaero, Yuseong-gu, Daejeon 34055, Republic of Korea
D. J. Eden
Affiliation:
Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK
L. V. Tóth
Affiliation:
Department of Astronomy, Eötvös Loránd University, 1/A Pázmány Péter sétány, 1117 Budapest, Hungary email: [email protected] Konkoly Observatory of the HAS, 15-17 Konkoly Thege Miklós út, 1121 Budapest, Hungary
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Abstract

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The Planck all-sky submillimetre observations have made it possible to study Galactic cold clumps in diverse environments, to probe dust properties and to examine the earliest stages of star formation. The TOP-SCOPE joint survey program aims to statistically study the evolution of molecular clouds and the initial conditions of star formation in a wide variety of environments. In this work we carry out an investigation of the 200 brightest compact sources detected by Planck.

Keywords

surveysISM: cloudsISM: abundancesstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S345: Origins: From the Protosun to the First Steps of Life , August 2018 , pp. 373 - 374
Copyright
© International Astronomical Union 2020 

References

Planck Collaboration 2016, A&A, 594, A28 Google Scholar
Liu, T. et al. 2018, ApJS, 234, 28L CrossRefGoogle Scholar
Eden, D. J. et al. 2017, MNRAS, 469, 2163E CrossRefGoogle Scholar