ISO ammonia line absorption reveals a layer of hot gas veiling Sgr B2-Reference-Cited by-同舟云学术

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ISO ammonia line absorption reveals a layer of hot gas veiling Sgr B2

Published:2002-02 Issue:2 Volume:383 Page:603-613
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Ceccarelli C.,Baluteau J.-P.,Walmsley M.,Swinyard B. M.,Caux E.,Sidher S. D.,Cox P.,Gry C.,Kessler M.,Prusti T.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20011765/pdf

Reference44 articles.

1. Molecular abundances and low-mass star formation. 1: Si- and S-bearing species toward IRAS 16293-2422

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3. Seeds of Life in Space (SOLIS). IX. Chemical Segregation of SO2 and SO toward the Low-mass Protostellar Shocked Region of L1157;The Astrophysical Journal;2020-06-10

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5. A Centimeter-wave Study of Methanol and Ammonia Isotopologues in Sgr B2(N): Physical and Chemical Differentiation between Two Hot Cores;The Astrophysical Journal;2018-12-18

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