Work

Deuteration as an evolutionary tracer in massive-star formation

Year: 2011

Type: article

Abstract: Context. Theory predicts, and observations confirm, that the column density ratio of a molecule containing D to its counterpart containing H can be used as an evolutionary tracer in the low-mass star formation process.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361/201116631

Authors: F. Fontani, A. Palau, P. Caselli, Á. Sánchez-Monge, M. J. Butler, J. C. Tan, I. Jiménez-Serra, G. Busquet, S. Leurini, M. Audard

Institutions: European Southern Observatory, Institut de Radioastronomie Millimétrique, Institute of Space Sciences, University of Leeds, Institut de Ciències del Cosmos, Universitat de Barcelona, University of Florida, Harvard University, Center for Astrophysics Harvard & Smithsonian, National Institute for Astrophysics, Max Planck Institute for Radio Astronomy, University of Geneva

Language: English

Topic: Astrophysics and Star Formation Studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funders: National Science Foundation, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Ministerio de Ciencia e Innovación, Science and Technology Facilities Council, European Social Fund

Awards: G1323383031, G1679186985, G1856229163, G4034454202, G4104599821, G536623562, G580951548, ESO Fellowship Programme for ALMA, On the birth and growth of young stars in molecular clouds, Disks around Young Stellar Objects

OpenAlex ID: W2120604812

FWCI: 4.929

Cites: 39

Cited by: 137

Related to: 10