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Connecting gas dynamics and star formation histories in nearby galaxies: the VLA—ANGST survey

Ott, Jürgen and Skillman, Evan and Dalcanton, Julianne and Walter, Fabian and Stilp, Adrienne and Koribalski, Bärbel and West, Andrew and Warren, Steven (2008) Connecting gas dynamics and star formation histories in nearby galaxies: the VLA—ANGST survey. In: The evolution of galaxies through the neutral hydrogen window. AIP Conference Proceedings. No.1035. American Institute of Physics , Melville, NY, pp. 105-111. ISBN 9780735405585. https://resolver.caltech.edu/CaltechAUTHORS:20090507-073538247

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Abstract

In recent years, HST revolutionized the field of star formation in nearby galaxies. Due to its high angular resolution it has now become possible to construct star formation histories of individual stellar populations on scales of a few arcseconds spanning a range of up to ~600 Myr. This method will be applied to the ANGST galaxies, a large HST volume limited survey to map galaxies up to distances of 3.5–4.0 Mpc (excluding the Local Group). The ANGST sample is currently followed-up by high, ~6" resolution VLA observations of neutral, atomic hydrogen (HI) in the context of VLA-ANGST, an approved Large VLA Project. The VLA resolution is well matched to that of the spatially resolved star formation history maps. The combination of ANGST and VLA-ANGST data will provide a new, promising approach to study essential fields of galaxy evolution such as the triggering of star formation, the feedback of massive stars into the interstellar medium, and the structure and dynamics of the interstellar medium.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1063/1.2973559DOIArticle
http://link.aip.org/link/?APCPCS/1035/105/1PublisherArticle
ORCID:
AuthorORCID
Ott, Jürgen0000-0001-8224-1956
Walter, Fabian0000-0003-4793-7880
Additional Information:© 2008 American Institute of Physics. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Subject Keywords:ISM: kinematics and dynamics, ISM: structure, galaxies: evolution. Stars: formation. galaxies: ISM, radio lines: ISM
Series Name:AIP Conference Proceedings
Issue or Number:1035
Classification Code:PACS: 95.55.Jz, 95.85.Bh, 98.38.Gt
Record Number:CaltechAUTHORS:20090507-073538247
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20090507-073538247
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:14173
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 May 2009 23:16
Last Modified:03 Oct 2019 00:47

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