activity
20142026
most citedA 2-3 billion year old major merger paradigm for the Andromeda galaxy and its outskirts

140 citations · 348 across the 15 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2026

A Self-Consistent Jeans Analysis of the Milky Way Rotation Curve

Yongjun Jiao, Francois Hammer, Istiak Akib +2

Jeans-based measurements of the Milky Way (MW) rotation curve (RC) have revealed a declining outer RC. The interpretation, however, depends sensitively on the tracer selection, the…

astro-ph.GA2026

Reconciling Galactic rotation curve constraints with stellar stream modeling

Mingyu Chang, Francois Hammer, Yanbin Yang

Recent Gaia-based measurements of the Milky Way rotation curve and stellar-stream modeling give significantly different estimates of the Galactic dynamical mass beyond Galactocentr…

astro-ph.GA2026

Ram-pressure signatures in the dwarf irregular galaxy SextansB revealed by deep MeerKAT HI observations

Brenda Namumba, Neel Kolhe, Francois Hammer +12

The impact of extremely low-density environments such as the diffuse intergalactic medium (IGM) on the neutral gas distribution of dwarf galaxies remains poorly explored observatio…

astro-ph.GA2026

Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group

Francois Hammer, Yanbin Yang

The discovery of dark matter-free (DM-free) dwarf galaxies in the NGC 1052 neighborhood has had a considerable impact on modern cosmology. The galaxies have been explained through…

astro-ph.GA2025

Young stars discovered in dwarf spheroidal galaxies confirm their recent infall into the Milky way

Francois Hammer, Piercarlo Bonifacio, Elisabetta Caffau +10

Recent observations from the ESA Gaia satellite and with the ESO VLT, have identified the presence of a population of young, 0.5 to 2 Gyr old, stars in the halo and in dwarf sphero…

astro-ph.GA2024★ 5 cited

Dark matter fraction derived from the M31 rotation curve

F. Hammer, Y. B. Yang, P. Amram +6

Mass estimates of a spiral galaxy derived from its rotation curve must account for the galaxy's past accretion history. There are several lines of evidence indicating that M31 expe…

astro-ph.GA2024★ 5 cited

The Milky Way accretion history compared to cosmological simulations -- from bulge to dwarf galaxy infall

F. Hammer, Y. J. Jiao, G. A. Mamon +6

Galactic halos are known to grow hierarchically, inside out. This implies a correlation between the infall lookback time of satellites and their binding energy. Cosmological simula…

astro-ph.GA2023

The Accretion History of the Milky Way: III. Hydrodynamical Simulations of Galactic Dwarf Galaxies at First Infall

Jianling Wang, Francois Hammer, Yanbin Yang +3

Most Milky Way dwarf galaxies are much less bound to their host than are relics of Gaia-Sausage-Enceladus and Sgr. These dwarfs are expected to have fallen into the Galactic halo l…

astro-ph.GA2023

The accretion history of the Milky Way. II. Internal kinematics of globular clusters and of dwarf galaxies

Francois Hammer, Jianling Wang, Gary A. Mamon +7

We study how structural properties of globular clusters and dwarf galaxies are linked to their orbits in the Milky Way halo. From the inner to the outer halo, orbital energy increa…

astro-ph.GA2023★ 2 cited

The discovery of the faintest known Milky Way satellite using UNIONS

Simon E. T. Smith, William Cerny, Christian R. Hayes +14

We present the discovery of Ursa Major III/UNIONS 1, the least luminous known satellite of the Milky Way, which is estimated to have an absolute V-band magnitude of $+2.2^{+0.4}_{-…

astro-ph.GA2023★ 102 cited

Detection of the Keplerian decline in the Milky Way rotation curve

Yongjun Jiao, Francois Hammer, Haifeng Wang +4

Our position inside the Galactic disc had prevented us from establishing an accurate rotation curve, until the advent of Gaia, whose third data release (Gaia DR3) made it possible…

astro-ph.GA2018★ 140 cited

A 2-3 billion year old major merger paradigm for the Andromeda galaxy and its outskirts

F. Hammer, Y. B. Yang, J. L. Wang +3

Recent observations of our neighbouring galaxy M31 have revealed that its disk was shaped by widespread events. The evidence for this includes the high dispersion ( 3) o…

astro-ph.GA2017★ 24 cited

Most pseudo-bulges can be formed at later stages of major mergers

T Sauvaget, F Hammer, M Puech +3

Most giant spiral galaxies have pseudo or disk-like bulges that are considered to be the result of purely secular processes. This may challenge the hierarchical scenario predicting…

astro-ph.GA2016★ 51 cited

Morpho-kinematics of z~1 galaxies probe the hierarchical scenario

M. Rodrigues, F. Hammer, H. Flores +2

We have studied a representative sample of intermediate-mass galaxies at z~1, observed by the kinematic survey KMOS3D. We have re-estimated the kinematical parameters from the publ…

astro-ph.IM2016★ 6 cited

The E-ELT Multi-Object Spectrograph: latest news from MOSAIC

F. Hammer, S. Morris, L. Kaper +9

There are 8000 galaxies, including 1600 at z larger than 1.6, which could be simultaneously observed in an E-ELT field of view of 40 sq. arcmin. A considerable fraction of astrophy…

astro-ph.IM2016★ 6 cited

Science Requirements and Trade-offs for the MOSAIC Instrument for the European ELT

C. J. Evans, M. Puech, M. Rodrigues +9

Building on the comprehensive White Paper on the scientific case for multi-object spectroscopy on the European ELT, we present the top-level instrument requirements that are being…

astro-ph.IM2014★ 7 cited

Science Case and Requirements for the MOSAIC Concept for a Multi-Object Spectrograph for the European Extremely Large Telescope

C. J. Evans, M. Puech, B. Barbuy +55

Over the past 18 months we have revisited the science requirements for a multi-object spectrograph (MOS) for the European Extremely Large Telescope (E-ELT). These efforts span the…