activity
20052024
most citedThe Ages of 55 Globular Clusters as Determined Using an Improved delta V_TO^HB Method Along with Color-Magnitude Diagram Constraints, and Their Implications for Broader Issues

490 citations · 2.6k across the 52 of their papers we have counts for

collaborators

52 papers

astro-ph.IM2024★ 12 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

astro-ph.GA2024★ 1 cited

From gas to stars: MUSEings on the internal evolution of IC 1613

S. Taibi, G. Battaglia, M. M. Roth +9

The kinematics and chemical composition of stellar populations of different ages provide crucial information about the evolution of a galaxy. We aim to provide such information for…

astro-ph.GA2023★ 15 cited

The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies

Alina Boecker, Nadine Neumayer, Annalisa Pillepich +4

We investigate the origin of stars in the innermost of galaxies spanning stellar masses of at using the cos…

astro-ph.GA2022★ 35 cited

Nuclear star cluster formation in star-forming dwarf galaxies

Katja Fahrion, Teodora-Elena Bulichi, Michael Hilker +7

Nuclear star clusters (NSCs) are massive star clusters found in all types of galaxies from dwarfs to massive galaxies. Recent studies show that while low-mass NSCs in dwarf galaxie…

astro-ph.GA2022★ 15 cited

A Deep View into the Nucleus of the Sagittarius Dwarf Spheroidal Galaxy with MUSE. III. Discrete multi-component population-dynamical models based on the Jeans equations

Nikolay Kacharov, Mayte Alfaro-Cuello, Nadine Neumayer +12

We present comprehensive multi-component dynamical models of M54 (NGC6715), the nuclear star cluster of the Sagittarius dwarf galaxy (Sgr), which is undergoing a tidal disruption i…

astro-ph.GA2022★ 42 cited

The stellar metallicity gradients of Local Group dwarf galaxies

S. Taibi, G. Battaglia, R. Leaman +5

Through a homogeneous analysis of spectroscopic literature data of red giant stars, we determine the radial metallicity profiles of 30 dwarf galaxies in the Local Group. We explore…

astro-ph.GA2022★ 32 cited

The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427

Ling Zhu, Glenn van de Ven, Ryan Leaman +16

We report the discovery of ancient massive merger events in the early-type galaxies NGC 1380 and NGC 1427, members of the Fornax galaxy cluster. Both galaxies have been observed by…

astro-ph.GA2021★ 34 cited

Disentangling the formation mechanisms of nuclear star clusters

Katja Fahrion, Ryan Leaman, Mariya Lyubenova +1

Nuclear star clusters (NSCs) are massive star clusters found ubiquitously in the centres of galaxies, from the dwarf regime to massive ellipticals and spirals. The fraction of nucl…

astro-ph.GA2021★ 13 cited

On the link between nuclear star cluster and globular cluster system mass, nucleation fraction and environment

Ryan Leaman, Glenn van de Ven

We present a simple model for the host mass dependence of the galaxy nucleation fraction (), the galaxy's nuclear star cluster (NSC) mass and the mass in its surviving glo…

astro-ph.GA2021

Once in a blue stream: Detection of recent star formation in the NGC 7241 stellar stream with MEGARA

David Martinez-Delgado, Santi Roca-Fabrega, Armando Gil de Paz +23

In this work we study the striking case of a narrow blue stream around the NGC 7241 galaxy and its foreground dwarf companion. We want to figure out if the stream was generated by…

astro-ph.GA2021★ 39 cited

Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass

Ling Zhu, Annalisa Pillepich, Glenn van de Ven +6

Galactic dynamical structures are fossil records of the assembly histories of galaxies. By analyzing the cosmological hydrodynamical simulation TNG50, we find that a dynamical stru…

astro-ph.GA2021★ 20 cited

Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane

Thomas A. Davison, Mark A. Norris, Ryan Leaman +3

Galaxy mergers are instrumental in dictating the final mass, structure, stellar populations, and kinematics of galaxies. Cosmological galaxy simulations indicate that the most mass…

astro-ph.GA2021★ 15 cited

Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo

Gigi Y. C. Leung, Ryan Leaman, Giuseppina Battaglia +4

We present multi-tracer dynamical models of the low mass (), isolated dwarf irregular galaxy WLM in order to simultaneously constrain the inner slope of the dark…

astro-ph.GA2020★ 14 cited

Globular Cluster Systems of Relic Galaxies

Karla A. Alamo-Martínez, Ana L. Chies-Santos, Michael A. Beasley +6

We analyse the globular cluster (GC) systems of a sample of 15 massive, compact early-type galaxies (ETGs), 13 of which have already been identified as good relic galaxy candidates…

astro-ph.GA2020★ 85 cited

The inside-out formation of nuclear discs and the absence of old central spheroids in barred galaxies of the TIMER survey

Adrian Bittner, Patricia Sánchez-Blázquez, Dimitri A. Gadotti +13

The centres of disc galaxies host a variety of structures built via both internal and external processes. In this study, we constrain the formation and evolution of these central s…

astro-ph.GA2020★ 104 cited

Kinematic signatures of nuclear discs and bar-driven secular evolution in nearby galaxies of the MUSE TIMER project

Dimitri A. Gadotti, Adrian Bittner, Jesus Falcon-Barroso +13

The central regions of disc galaxies hold clues to the processes that dominate their formation and evolution. The TIMER project has obtained high signal-to-noise and spatial resolu…

astro-ph.GA2020★ 1 cited

Reconstructing the mass accretion histories of nearby Red Nuggets with their globular cluster systems

Michael A. Beasley, Ryan Leaman, Ignacio Trujillo +6

It is generally recognized that massive galaxies form through a combination of in-situ collapse and ex-situ accretion. The in-situ component forms early, where gas collapse and com…

astro-ph.GA2020★ 15 cited

Recovering age-metallicity distributions from integrated spectra: validation with MUSE data of a nearby nuclear star cluster

A. Boecker, M. Alfaro-Cuello, N. Neumayer +2

Current instruments and spectral analysis programs are now able to decompose the integrated spectrum of a stellar system into distributions of ages and metallicities. The reliabili…

astro-ph.GA2020★ 44 cited

Disentangling the formation history of galaxies via population-orbit superposition: method validation

Ling Zhu, Glenn van de Ven, Ryan Leaman +9

We present population-orbit superposition models for external galaxies based on Schwarzschild's orbit-superposition method, by tagging the orbits with age and metallicity. The mode…

astro-ph.GA2019★ 35 cited

A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph

Gigi Y. C. Leung, Ryan Leaman, Glenn van de Ven +1

The five globular clusters (GCs) of the Fornax dSph are puzzling for two reasons; the mass in GCs is high with respect to the galaxy's old stellar mass, and their survival and larg…

astro-ph.GA2019★ 51 cited

Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM

Saundra M. Albers, Daniel R. Weisz, Andrew A. Cole +11

We present the star formation history (SFH) of the isolated (D~970 kpc) Local Group dwarf galaxy WLM measured from color-magnitude diagrams constructed from deep Hubble Space Teles…

astro-ph.GA2019★ 21 cited

Is There a Fundamental Upper Limit to the Mass of a Star Cluster?

Mark A. Norris, Glenn van de Ven, Sheila J. Kannappan +2

The discovery around the turn of the millenium of a population of very massive (M > 210 M) compact stellar systems (CSS) with physical properties (radiu…

astro-ph.GA2019★ 27 cited

Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA

Ryan Leaman, Francesca Fragkoudi, Miguel Querejeta +15

Stellar feedback plays a significant role in modulating star formation, redistributing metals, and shaping the baryonic and dark structure of galaxies -- however, the efficiency of…

astro-ph.GA2019★ 39 cited

Constraining nuclear star cluster formation using MUSE-AO observations of the early-type galaxy FCC47

Katja Fahrion, Mariya Lyubenova, Glenn van de Ven +12

Nuclear star clusters (NSCs) are found in at least 70% of all galaxies, but their formation path is still unclear. In the most common scenarios, NSCs form in-situ from the galaxy's…