Chemical evolution in high-mass star-forming regions: Results from the malt90 survey › Research Explorer

Chemical evolution in high-mass star-forming regions: Results from the malt90 survey

Research output: Contribution to journal › Article › peer-review

DOI

https://doi.org/10.1088/0004-637X/777/2/157
Final published version

Sadia Hoq
James M. Jackson
Jonathan B. Foster
Patricio Sanhueza
Andrés Guzmán
J. S. Whitaker
Christopher Claysmith
Jill M. Rathborne
Tatiana Vasyunina
Anton Vasyunin

Original language	English
Article number	157
Number of pages	15
Journal	Astrophysical Journal
Volume	777
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/777/2/157
Publication status	Published - 10 Nov 2013

ASJC Scopus subject areas

Nuclear and High Energy Physics
Space and Planetary Science
Astronomy and Astrophysics

WoS ResearchAreas Categories

Astronomy & Astrophysics

Research areas

astrochemistry, ISM: abundances, ISM: clouds, ISM: molecules, stars: formation, INFRARED DARK CLOUDS, INTERSTELLAR MOLECULAR CLOUDS, COLLAPSING PRESTELLAR CORES, PROTOSTELLAR CORES, ABUNDANCE RATIO, MILKY-WAY, GALACTIC PLANE, HNC, HCN, CHEMISTRY

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