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20172024
most citedConnection Between Stellar Mass Distributions Within Galaxies and Quenching Since z =2

89 citations · 138 across the 4 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA20249 cited

WEAVE First Light Observations: Origin and Dynamics of the Shock Front in Stephan's Quintet

M. I. Arnaudova, S. Das, D. J. B. Smith +62

We present a detailed study of the large-scale shock front in Stephan's Quintet, a byproduct of past and ongoing interactions. Using integral-field spectroscopy from the new Willia…

astro-ph.GA202118 cited

The Isaac Newton Telescope monitoring survey of Local Group dwarf galaxies -- IV. The star formation history of Andromeda VII derived from long period variable stars

Mahdieh Navabi, Elham Saremi, Atefeh Javadi +10

We have examined the star formation history (SFH) of Andromeda VII (And VII), the brightest and most massive dwarf spheroidal (dSph) satellite of the Andromeda galaxy (M 31). Altho…

astro-ph.GA202022 cited

The Isaac Newton Telescope monitoring survey of Local Group dwarf galaxies. I. Survey overview and first results for Andromeda I

Elham Saremi, Atefeh Javadi, Jacco Th. van Loon +10

An optical monitoring survey in the nearby dwarf galaxies was carried out with the 2.5-m Isaac Newton Telescope (INT). 55 dwarf galaxies and four isolated globular clusters in the…

astro-ph.GA2018

The number of dwarf satellites of disk galaxies versus their bulge mass in the standard model of cosmology

B. Javanmardi, M. Raouf, H. G. Khosroshahi +3

There is a correlation between bulge mass of the three main galaxies of the Local Group (LG), i.e. M31, Milky Way (MW), and M33, and the number of their dwarf spheroidal galaxies.…

astro-ph.GA201789 cited

Connection Between Stellar Mass Distributions Within Galaxies and Quenching Since z =2

Moein Mosleh, Sandro Tacchella, Alvio Renzini +5

We study the history from to of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose we use multi-wa…