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19932026
most citedMILES: A Medium resolution INT Library of Empirical Spectra

1.6k citations · 12.4k across the 179 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

9 papers · 2 filters

astro-ph.GA2019★ 57 cited

The CALIFA view on stellar angular momentum across the Hubble sequence

J. Falcón-Barroso, G. van de Ven, M. Lyubenova +32

[Abridged] We present the apparent stellar angular momentum of 300 galaxies across the Hubble sequence, using integral-field spectroscopic data from the CALIFA survey. Adopting the…

astro-ph.GA2019★ 19 cited

Leavers and remainers: Galaxies split by group-exit

Nelvy Choque-Challapa, Rory Smith, Graeme Candlish +2

The disruption of substructure in galaxy clusters likely plays an important role in shaping the cluster population as a significant fraction of cluster galaxies today have spent ti…

astro-ph.GA2019★ 42 cited

A spectroscopic census of the Fornax cluster and beyond: preparing for next generation surveys

Natasha Maddox, Paolo Serra, Aku Venhola +3

The Fornax cluster is the nearest, large cluster in the southern sky, and is currently experiencing active assembly of mass. It is thus the target of a number of ongoing observing…

astro-ph.GA2019★ 30 cited

Neutral hydrogen gas within and around NGC 1316

P. Serra, F. M. Maccagni, D. Kleiner +20

We present MeerKAT observations of neutral hydrogen gas (HI) in the nearby merger remnant NGC 1316 (Fornax A), the brightest member of a galaxy group which is falling into the Forn…

astro-ph.GA2019★ 29 cited

Young stellar populations in early-type dwarf galaxies; occurrence, radial extent and scaling relations

Elaheh Hamraz, Reynier F. Peletier, Habib Khosroshahi +3

To understand the stellar population content of dwarf early-type galaxies (dEs) and its environmental dependence, we compare the slopes and intrinsic scatter of color-magnitude rel…

astro-ph.GA2019★ 29 cited

The kinematics of local thick discs do not support an accretion origin

Sébastien Comerón, Heikki Salo, Johan H. Knapen +1

Thick discs are nearly ubiquitous components of the discs of present-day galaxies. It has been proposed that a fraction of their stars has been accreted. Here, we aim to find wheth…