Log in to save to my catalogue

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

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2365913050

The Satellite Luminosity Function of M101 into the Ultra-Faint Dwarf Galaxy Regime

About this item

Full title

The Satellite Luminosity Function of M101 into the Ultra-Faint Dwarf Galaxy Regime

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-03

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

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

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

How to access this item