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Nearby Halo Streams

Grillmair, Carl J. (2014) Nearby Halo Streams. In: Lessons from the Local Group: A Conference in honour of David Block and Bruce Elmegreen. Springer , Cham, pp. 365-377. ISBN 978-3-319-10614-4. https://resolver.caltech.edu/CaltechAUTHORS:20170616-134406214

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Abstract

The number of known halo streams has increased dramatically with the advent of deep, well-calibrated, wide-area sky surveys. Twenty nearby halo streams have been discovered to date, a number that is likely to at least double as surveys of the southern hemisphere progress. By themselves these streams tell us something about the accretion and disruption history of stellar aggregates in our Galaxy. More importantly, they will ultimately enable us to put much tighter constraints on the three dimensional shape of the Galactic potential. The morphologies of cold streams may also help us to constrain the occurrence and mass function of a predicted population of dark matter subhalos. We tabulate some basic properties of the known nearby streams, and discuss prospects for future discoveries.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://dx.doi.org/10.1007/978-3-319-10614-4_30DOIArticle
http://rdcu.be/twhOPublisherFree ReadCube access
ORCID:
AuthorORCID
Grillmair, Carl J.0000-0003-4072-169X
Additional Information:© 2015 Springer International Publishing Switzerland. First Online: 14 November 2014.
Group:Infrared Processing and Analysis Center (IPAC)
Record Number:CaltechAUTHORS:20170616-134406214
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170616-134406214
Official Citation:Grillmair C. (2015) Nearby Halo Streams. In: Freeman K., Elmegreen B., Block D., Woolway M. (eds) Lessons from the Local Group. Springer, Cham
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:78289
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:16 Jun 2017 20:57
Last Modified:29 Apr 2020 19:48

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