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

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Showing astro-ph.COShow all

6 papers · 1 filter

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.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.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…