Tracing the Formation History of Giant Planets in Protoplanetary Disks with Carbon, Oxygen, Nitrogen, and Sulfur-Reference-Cited by-同舟云学术

Tracing the Formation History of Giant Planets in Protoplanetary Disks with Carbon, Oxygen, Nitrogen, and Sulfur

Published:2021-03-01 Issue:1 Volume:909 Page:40
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Turrini D.^ORCID,Schisano E.^ORCID,Fonte S.^ORCID,Molinari S.^ORCID,Politi R.^ORCID,Fedele D.^ORCID,Panić O.^ORCID,Kama M.^ORCID,Changeat Q.^ORCID,Tinetti G.^ORCID

Funder

Science and Technology Funding Council

Italian Space Agency

National Institute of Astrophysics

University of Tartu - ASTRA project

European Research Council

Royal Society Dorothy Hodgkin Fellowship

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abd6e5/pdf

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2. Cometary Chemistry and the Origin of Icy Solar System Bodies: The View After Rosetta

3. The Disk Substructures at High Angular Resolution Project (DSHARP). I. Motivation, Sample, Calibration, and Overview

4. ALMA Survey of Lupus Protoplanetary Disks. II. Gas Disk Radii

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