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An observational survey of protoplanetary carbon in young stellar systems across the galaxy

Smith, R. L. and Blake, G. A. and Boogert, A. C. A. and Pontoppidan, K. M. (2017) An observational survey of protoplanetary carbon in young stellar systems across the galaxy. Meteoritics and Planetary Science, 52 (S1). Art. No. A330. ISSN 1086-9379. https://resolver.caltech.edu/CaltechAUTHORS:20180122-155851410

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Abstract

High-resolution near-infrared absorption spectroscopy of the rovibrational transitions of carbon monoxide (CO) gas toward young stellar objects (YSOs) enables precise evaluation of carbon and oxygen isotopes in these systems, providing insight into protoplanetary processes [1-6]. Meaningful comparisons can be made between solar system materials and young stellar gas, furthering our understanding of phenomena that could have affected chemistry in the early solar nebula, including CO self-shielding [3,6], supernova enrichment [4], and interplay between ^(12)C^(16)O ice and gas reservoirs [5,6]. Such data also enable the assessment of potential differences in chemical pathways between isolated cores and low-mass binary systems separated within a few hundred AU [5].


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1111/maps.12934DOIAbstracts
http://onlinelibrary.wiley.com/doi/10.1111/maps.12934/abstractPublisherAbstracts
ORCID:
AuthorORCID
Blake, G. A.0000-0003-0787-1610
Pontoppidan, K. M.0000-0001-7552-1562
Additional Information:© 2017 Meteoritical Society. First published: 6 July 2017.
Group:Astronomy Department
Issue or Number:S1
Record Number:CaltechAUTHORS:20180122-155851410
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180122-155851410
Official Citation:(2017), 80th Annual Meeting of the Meteoritical Society (2017). Meteorit Planet Sci, 52: A1–A408. doi:10.1111/maps.12934
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84464
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:23 Jan 2018 13:19
Last Modified:20 Apr 2020 08:47

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