activity
20092024
most citedGRB 100219A with X-shooter - abundances in a galaxy at z = 4.7

100 citations · 509 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2024

The accretion history of the Milky Way IV. Hints of recent star formation in Milky Way dwarf spheroidal galaxies

Yanbin Yang, Elisabetta Caffau, Piercarlo Bonifacio +3

Dwarf spheroidal galaxies are known to be dominated by old stellar populations. This has led to the assumption that their gas-rich progenitors lost their gas during their infall in…

astro-ph.GA2023

Gaia EDR3 proper motions, energies, angular momenta of Milky Way dwarf galaxies: a recent infall to the Milky Way halo

Yang Y., Hammer F., Li H. +7

Gaia EDR3 has provided proper motions of Milky Way (MW) dwarf galaxies with an unprecedented accuracy, which allows us to investigate their orbital properties. We found that the to…

astro-ph.GA2021★ 9 cited

Kinematical asymmetry in the dwarf irregular galaxy WLM and a perturbed halo potential

M. Khademi, Y. Yang, F. Hammer +1

WLM is a dwarf irregular that is seen almost edge-on that has prompted a number of kinematical studies investigating its rotation curve and its dark matter content. In this paper,…

astro-ph.GA2020★ 19 cited

Lyman continuum leakage in faint star-forming galaxies at redshift z=3-3.5 probed by gamma-ray bursts

J. -B. Vielfaure, S. D. Vergani, J. Japelj +23

We present the observations of Lyman continuum (LyC) emission in the afterglow spectra of GRB 191004B at , together with those of the other two previously known LyC-emitt…

astro-ph.HE2019★ 1 cited

Outflows from GRB hosts are ubiquitous: Kinematics of z<0.3 GRB-SN hosts resolved with FLAMES

C. C. Thöne, L. Izzo, H. Flores +12

The hosts of long duration gamma-ray bursts are predominantly starburst galaxies at subsolar metallicity. At redshifts z<1, this implies that most of them are low-mass galaxies sim…

astro-ph.GA2013★ 51 cited

X-Shooter GTO: evidence for a population of extremely metal-poor, alpha-poor stars

E. Caffau, P. Bonifacio, P. Francois +12

The extremely metal-poor stars are the direct descendants of the first generation stars. They carry the chemical signature of the pristine Universe at the time they formed, shortly…

astro-ph.CO2013★ 53 cited

Spectroscopy of the short-hard GRB 130603B: The host galaxy and environment of a compact object merger

A. de Ugarte Postigo, C. C. Thoene, A. Rowlinson +40

Short duration gamma-ray bursts (SGRBs) are thought to be related to the violent merger of compact objects, such as neutron stars or black holes, which makes them promising sources…

astro-ph.CO2013★ 35 cited

Modelling narrow-line regions of active galaxies in the Sloan Digital Sky Survey - I.Sample selection and physical conditions

Zhitai Zhang, Yanchun Liang, François Hammer

We systematically determine the electron density and electron temperature of active galaxies and star-forming galaxies using spectroscopy from the SDSS DR7, while mainly focusing o…

astro-ph.CO2012

A possible impact near the Milky Way of a former major merger in the Local Group

Sylvain Fouquet, François Hammer, Yanbin Yang +2

The Milky Way (MW) dwarf system presents two exceptional features, namely it forms a thick plane called the Vast Polar Structure (VPOS), and the two biggest dwarves, the Magellanic…

astro-ph.GA2012★ 69 cited

Does the dwarf galaxy system of the Milky Way originate from Andromeda?

Sylvain Fouquet, François Hammer, Yanbin Yang +2

The Local Group is often seen to be a quiescent environment without significant merger events. However an ancient major merger may have occurred in the most massive galaxy. Numeric…

astro-ph.CO2012★ 68 cited

Galaxy disks do not need to survive in the L-CDM paradigm: the galaxy merger rate out to z~1.5 from morpho-kinematic data

M. Puech, F. Hammer, P. F. Hopkins +5

About two-thirds of present-day, large galaxies are spirals such as the Milky Way or Andromeda, but the way their thin rotating disks formed remains uncertain. Observations have re…

astro-ph.HE2012★ 100 cited

GRB 100219A with X-shooter - abundances in a galaxy at z = 4.7

C. C. Thoene, J. P. U. Fynbo, P. Goldoni +24

Abundances of galaxies at redshifts z > 4 are difficult to obtain from damped Ly α (DLA) systems in the sightlines of quasars (QSOs) due to the Ly α forest blanketing and the low n…

astro-ph.CO2012★ 27 cited

A decrease of the gas exchanges between galaxies and the IGM, from 12 to 6 billion years ago

M. Rodrigues, M. Puech, F. Hammer +2

Using a representative sample of 65 intermediate mass galaxies at z \sim 0.6, we have inves- tigated the interplay between the main ingredients of chemical evolution: metal abundan…

astro-ph.CO2011★ 3 cited

Could M31 be the result of a major merger?

Sylvain Fouquet, François Hammer, Yang-Bin Yang +3

We investigated a scenario in which M31 could be the remnant of a gas-rich major merger. Galaxy merger simulations, highly constrained by observations, were run using GADGET 2 in o…

astro-ph.SR2011★ 18 cited

Extremely metal-poor stars in SDSS fields

Piercarlo Bonifacio, Elisabetta Caffau, Patrick François +12

Some insight on the first generation of stars can be obtained from the chemical composition of their direct descendants, extremely metal-poor stars (EMP), with metallicity less tha…

astro-ph.GA2010★ 29 cited

Could the Magellanic Clouds be tidal dwarves expelled from a past-merger event occurring in Andromeda?

Yanbin YANG, Francois HAMMER

The Magellanic Clouds are often considered as outliers in the satellite system of the Milky Way because they are irregular and gas-rich galaxies. From their large relative motion,…

astro-ph.HE2009★ 27 cited

GRB 090313: X-shooter's first shot at a GRB

A. de Ugarte Postigo, P. Goldoni, C. C. Thöne +26

Context. X-shooter is the first second-generation instrument to become operative at the ESO Very Large Telescope (VLT). It is a broad-band medium-resolution spectrograph designed w…