The Satellite Luminosity Function of M101 into the Ultra-Faint Dwarf Galaxy Regime
The Satellite Luminosity Function of M101 into the Ultra-Faint Dwarf Galaxy Regime
About this item
Full title
Author / Creator
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
We have obtained deep Hubble Space Telescope (HST) imaging of four faint and ultra-faint dwarf galaxy candidates in the vicinity of M101 - Dw21, Dw22, Dw23 and Dw35, originally discovered by Bennet et al. (2017). Previous distance estimates using the surface brightness fluctuation technique have suggested that these four dwarf candidates are the on...
Alternative Titles
Full title
The Satellite Luminosity Function of M101 into the Ultra-Faint Dwarf Galaxy Regime
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2365913050
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2365913050
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2002.11126