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The Nature of Low-Density Star Formation

Thilker, David and Lee, Janice and Capak, Peter and Cook, David and Dale, Daniel and Elmegreen, Bruce and Gil de Paz, Armando and Gallagher, John and Hunter, Deidre and Leroy, Adam and Meurer, Gerhardt and Pisano, D. J. and Rafelski, Marc and Tosi, Monica and Wofford, Aida (2019) The Nature of Low-Density Star Formation. Astro2020 Science White Paper, . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20190812-144155775

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Abstract

How do stars manage to form within low-density, HI-dominated gas? Such environments provide a laboratory for studying star formation with physical conditions distinct from starbursts and the metal-rich disks of spiral galaxies where most effort has been invested. Here we outline fundamental open questions about the nature of star formation at low-density. We describe the wide-field, high-resolution UV-optical-IR-radio observations of stars, star clusters and gas clouds in nearby galaxies needed in the 2020's to provide definitive answers, essential for development of a complete theory of star formation.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1903.05745arXivDiscussion Paper
ORCID:
AuthorORCID
Thilker, David0000-0002-8528-7340
Lee, Janice0000-0002-2278-9407
Capak, Peter0000-0003-3578-6843
Cook, David0000-0002-6877-7655
Dale, Daniel0000-0002-5782-9093
Elmegreen, Bruce0000-0002-1723-6330
Gil de Paz, Armando0000-0001-6150-2854
Hunter, Deidre0000-0002-3322-9798
Leroy, Adam0000-0002-2545-1700
Meurer, Gerhardt0000-0002-0163-2507
Rafelski, Marc0000-0002-9946-4731
Group:Infrared Processing and Analysis Center (IPAC)
Series Name:Astro2020 Science White Paper
Record Number:CaltechAUTHORS:20190812-144155775
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190812-144155775
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97794
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:12 Aug 2019 22:23
Last Modified:09 Mar 2020 13:19

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