activity
20012011
most citedLocal kinematics of K and M giants from Coravel/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters

440 citations · 801 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2011★ 119 cited

Overlapping abundance gradients and azimuthal gradients related to the spiral structure of the Galaxy

J. R. D. Lepine, P. Cruz, S. Scarano +6

The connection between some features of the metallicity gradient in the Galactic disk, best revealed by Open Clusters and Cepheids, and the spiral structure, is explored. The step-…

astro-ph.GA2011★ 67 cited

Chemically tagging the Hyades stream: Does it partly originate from the Hyades cluster?

L. Pompéia, T. Masseron, B. Famaey +19

The Hyades stream has long been thought to be a dispersed vestige of the Hyades cluster. However, recent analyses of the parallax distribution, of the mass function, and of the act…

astro-ph.GA2009★ 50 cited

Galactic kinematics with modified Newtonian dynamics

O. Bienaymé, B. Famaey, X. Wu +2

We look for observational signatures that could discriminate between Newtonian and modified Newtonian (MOND) dynamics in the Milky Way, in view of the advent of large astrometric a…

astro-ph.SR2009★ 7 cited

Spectroscopic binaries among Hipparcos M giants II. Binary frequency

A. Frankowski, B. Famaey, S. Van Eck +3

This paper is the second one in a series devoted to the study of properties of binaries involving M giants. The binary frequency of field M giants is derived and compared with the…

astro-ph2007★ 4 cited

The wedding of modified dynamics and non-exotic dark matter in galaxy clusters

B. Famaey, G. W. Angus, G. Gentile +2

We summarize the status of Modified Newtonian Dynamics (MOND) in galaxy clusters. The observed acceleration is typically larger than the acceleration threshold of MOND in the centr…

astro-ph2006★ 101 cited

The Hyades stream: evaporated cluster or intrusion from the inner disk?

B. Famaey, F. Pont, X. Luri +3

The nature of the Hyades stream, or Hyades moving group, is a long-standing question of Galactic Astronomy. Is this stream caused by non-axisymmetric perturbations of the galactic…