Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· arXiv e-print (arXiv:0708.1523)
· References in the article
· Citations to the Article (2) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Chemical complexity in galaxies
Authors:
Turner, Jean L.; Meier, David S.
Affiliation:
AA(Department of Physics and Astronomy, UCLA), AB(Jansky Fellow, NRAO)
Publication:
Astrophysics and Space Science, Volume 313, Issue 1-3, pp. 267-272 (Ap&SS Homepage)
Publication Date:
01/2008
Origin:
SPRINGER
Keywords:
Galaxies: ISM, Astrochemistry, Galaxies: individual (IC 342, M 82)
DOI:
10.1007/s10509-007-9633-2
Bibliographic Code:
2008Ap&SS.313..267T

Abstract

ALMA will be able to detect a broad spectrum of molecular lines in galaxies. Current observations indicate that the molecular line emission from galaxies is remarkably variable, even on kpc scales. Imaging spectroscopy at resolutions of an arcsecond or better will reduce the chemical complexity by allowing regions of physical conditions to be defined and classified.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints