Author
Listed:
- Sandra Brünken
(I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany)
- Olli Sipilä
(PO Box 64, 00014 University of Helsinki
Max-Planck Institut für Extraterrestrische Physik, Gießenbachstraße 1, 85741 Garching bei München, Germany)
- Edward T. Chambers
(I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany)
- Jorma Harju
(PO Box 64, 00014 University of Helsinki)
- Paola Caselli
(Max-Planck Institut für Extraterrestrische Physik, Gießenbachstraße 1, 85741 Garching bei München, Germany
School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK)
- Oskar Asvany
(I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany)
- Cornelia E. Honingh
(I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany)
- Tomasz Kamiński
(Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany)
- Karl M. Menten
(Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany)
- Jürgen Stutzki
(I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany)
- Stephan Schlemmer
(I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany)
Abstract
Observations of emission and absorption lines of the deuterated trihydrogen cation (H2D+) from a dense interstellar cloud core, combined with chemical modelling, reveal that the core needed at least one million years to form Sun-like stars.
Suggested Citation
Sandra Brünken & Olli Sipilä & Edward T. Chambers & Jorma Harju & Paola Caselli & Oskar Asvany & Cornelia E. Honingh & Tomasz Kamiński & Karl M. Menten & Jürgen Stutzki & Stephan Schlemmer, 2014.
"H2D+ observations give an age of at least one million years for a cloud core forming Sun-like stars,"
Nature, Nature, vol. 516(7530), pages 219-221, December.
Handle:
RePEc:nat:nature:v:516:y:2014:i:7530:d:10.1038_nature13924
DOI: 10.1038/nature13924
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