Full-spectral fitting techniques to characterise the stellar content of ultra diffuse galaxies
Full-spectral fitting techniques to characterise the stellar content of ultra diffuse galaxies
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Language
English
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Contents
Understanding the peculiar properties of Ultra Diffuse Galaxies (UDGs) via spectroscopic analysis is a challenging task that is now becoming feasible. The advent of 10m-class telescopes and high sensitivity instruments is enabling the gathering of high quality spectra even for the faintest systems. In addition, advances in the modelling of stellar...
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Full title
Full-spectral fitting techniques to characterise the stellar content of ultra diffuse galaxies
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TN_cdi_crossref_primary_10_1017_S174392131800577X
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_crossref_primary_10_1017_S174392131800577X
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ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S174392131800577X
