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Journal ArticleDOI

High-Resolution Mapping of Molecular Outflows in NGC 2071, W49, and NGC 7538

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TLDR
In this article, the authors present des cartes de haute resolution (7'') du gaz moleculaire and de l'emission continue dans les noyaux de NGC 2071, W 49 and NGC 7538.
Abstract
On presente des cartes de haute resolution (7'') du gaz moleculaire et de l'emission continue dans les noyaux de NGC 2071, W 49 et NGC 7538. Les masses du gaz de haute vitesse, detecte par l'interferometre, sont respectivement de 0,2; 138 et 12 M ○. . L'emission continue a 2,7 mm a ete detectee dans toutes les sources

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Journal ArticleDOI

Massive Stars : Their Environment and Formation

TL;DR: In this paper, the physical characteristics of the environment around recently formed massive stars are reviewed and a large body of data, gathered during the last decade, has allowed signi cant progress in the understanding of the physical processes that take place during the formation and early evolution of massive stars.
Journal ArticleDOI

A HIGH-RESOLUTION STUDY OF GAS AND DUST AROUND YOUNG INTERMEDIATE-MASS STARS: EVIDENCE FOR CIRCUMSTELLAR DISKS IN HERBIG Ae SYSTEMS

TL;DR: In this paper, the environments of seven pre-main-sequence stars of spectral type Ae using millimeter-wave continuum and molecular line aperture synthesis imaging were probed using a long-term program of observations to search for and characterize disks of gas and dust.
Journal ArticleDOI

H2 and CO Emission from Disks around T Tauri and Herbig Ae Pre-Main-Sequence Stars and from Debris Disks around Young Stars: Warm and Cold Circumstellar Gas*

TL;DR: In this article, ISO Short-Wavelength Spectrometer observations of H 2 pure-rotational line emission from the disks around low and intermediate-mass pre-main-sequence stars as well as from young stars thought to be surrounded by debris disks are presented.
Journal ArticleDOI

Envelope structure on 700 AU scales and the molecular outflows of low-mass young stellar objects

TL;DR: Trends support the hypothesis that outflows are driven by accretion through a disk, with a global mass infall rate determined by the mass and density of the envelope.
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