Version: 6.3

WATER VAPOR IN THE INNER 25 AU OF A YOUNG DISK AROUND A LOW-MASS PROTOSTAR*

Author

Jes K. Jørgensen1,4 and Ewine F. van Dishoeck2,3

Affiliations

1 Argelander-Institut für Astronomie, University of Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
2 Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, The Netherlands
3 Max-Planck Institut für extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany
4 Current address: Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5-7, DK-1350 Copenhagen K, Denmark.

E-mail

jes@snm.ku.dk ewine@strw.leidenuniv.nl

Journal

The Astrophysical Journal Letters Create an alert RSS this journal

Issue

Volume 710, Number 1

Citation

Jes K. Jørgensen and Ewine F. van Dishoeck 2010 ApJ 710 L72

doi: 10.1088/2041-8205/710/1/L72


 
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ABSTRACT

Water is one of the key molecules in the physical and chemical evolution of star- and planet-forming regions. We here report the first spatially resolved observation of thermal emission of (an isotopologue of) water with the Plateau de Bure Interferometer toward the deeply embedded Class 0 protostar NGC 1333-IRAS4B. The observations of the H18 2O 31,3-22,0 transition at 203.4 GHz resolve the emission of water toward this source with an extent of about 0farcs2 corresponding to the inner 25 AU (radius). The H18 2O emission reveals a tentative velocity gradient perpendicular to the extent of the protostellar outflow/jet probed by observations of CO rotational transitions and water masers. The line is narrow, ≈1 km s–1 (FWHM), significantly less than what would be expected for emission from an infalling envelope or accretion shock, but consistent with emission from a disk seen at a low inclination angle. The water column density inferred from these data suggests that the water emitting gas is a thin warm layer containing about 25 M Earth of material, 0.03% of the total disk mass traced by continuum observations.

Footnote
*  Based on observations carried out with the Institut de Radioastronomie Millimétrique (IRAM) Plateau de Bure Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain).
Subject headings

astrochemistry; ISM: abundances; ISM: individual objects (NGC 1333-IRAS4B); protoplanetary disks; stars: formation


PACS

97.21.+a Pre-main sequence objects, young stellar objects (YSO's) and protostars (T Tauri stars, Orion population, Herbig–Haro objects, Bok globules, bipolar outflows, cometary nebulae, etc.)

98.38.Bn Atomic, molecular, and chemical, and grain processes

98.38.Er Interstellar masers

97.10.Fy Circumstellar shells, clouds, and expanding envelopes; circumstellar masers

Subjects

Atomic and molecular physics

Astrophysics and astroparticles

Dates

Issue 1 (2010 February 10)

Received 2009 October 18 , accepted for publication 2010 January 7

Published 2010 January 22



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