TheHerschel/PACS view of the Cep OB2 region: Global protoplanetary disk evolution and clumpy star formation

2014/10/10 by Aurora Sicilia-Aguilar, A. Sicilia‐Aguilar, V. Roccatagliata +14
Chemistry · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Geology #Molecular Spectroscopy and Structure #Paleontology #Physics #Planet #Protoplanetary disk #Star (game theory) #Star formation #Stars #Stellar, planetary, and galactic studies #astro-ph.EP #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201424669

published as A&A 573, A19 (2015) · Accepted by A\&A. 18 pages plus Appendix with figures and tables

arxiv created 2014/10/10 · openalex publication_date 2014/10/21 · arxiv updated 2014/12/10 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The Cep OB2 region, with its two intermediate-aged clusters Tr 37 and NGC 7160, is a paradigm of sequential star formation and an ideal site for studies of protoplanetary disk evolution.

Citations

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