Millimeter Interferometry of Class 0 Sources: Rotation and Infall towards L1448N

Terebey, Susan; Padgett, Deborah L.

doi:10.1007/978-94-011-5608-0_42

Millimeter Interferometry of Class 0 Sources: Rotation and Infall towards L1448N

Susan Terebey³ &
Deborah L. Padgett⁴

Conference paper

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22 Citations

Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 182))

Abstract

In order to study the kinematics of protostellar collapse we present high-spatial resolution millimeter interferometer data of the class 0 source L1448 N. The L1448 N cloud core has fragmented into two rapidly rotating subcores containing three protostars. One subcore is a protobinary system with 2000 AU separation. Strong evidence for infall is seen towards the N(B) component.

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Authors and Affiliations

Extrasolar Research Corporation, 720 Magnolia Ave., Pasadena, CA, 91106, USA
Susan Terebey
Jet Propulsion Laboratory, IPAC 100-22, Caltech, Pasadena, CA, 91125, USA
Deborah L. Padgett

Authors

Susan Terebey
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Deborah L. Padgett
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Editor information

Editors and Affiliations

Observatoire de Grenoble, France
Bo Reipurth
Institut d’Astrophysique de Paris, France
Claude Bertout

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Terebey, S., Padgett, D.L. (1997). Millimeter Interferometry of Class 0 Sources: Rotation and Infall towards L1448N. In: Reipurth, B., Bertout, C. (eds) Herbig-Haro Flows and the Birth of Low Mass Stars. International Astronomical Union / Union Astronomique Internationale, vol 182. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5608-0_42

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DOI: https://doi.org/10.1007/978-94-011-5608-0_42
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-4661-6
Online ISBN: 978-94-011-5608-0
eBook Packages: Springer Book Archive

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