An old disk still capable of forming a planetary system View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2013-01-30

AUTHORS

Edwin A. Bergin, L. Ilsedore Cleeves, Uma Gorti, Ke Zhang, Geoffrey A. Blake, Joel D. Green, Sean M. Andrews, Neal J. Evans II, Thomas Henning, Karin Öberg, Klaus Pontoppidan, Chunhua Qi, Colette Salyk, Ewine F. van Dishoeck

ABSTRACT

In combination with existing observations and detailed circumstellar models, the detection of hydrogen deuteride emission from the star TW Hydrae implies a circumstellar disk mass of more than 0.05 solar masses, which is enough to form a planetary system like our own.

PAGES

644-646

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature11805

DOI

http://dx.doi.org/10.1038/nature11805

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1034582520

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/23364742


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