output
20022015
most citedDiscrete Hierarchical Organization of Social Group Sizes

585 citations

Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA201566 cited

The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc

G. R. Ruchti, J. I. Read, S. Feltzing +26

According to our current cosmological model, galaxies like the Milky Way are expected to experience many mergers over their lifetimes. The most massive of the merging galaxies will…

astro-ph.GA201485 cited

The first carbon-enhanced metal-poor star found in the Sculptor dwarf spheroidal

Asa Skuladottir, Eline Tolstoy, Stefania Salvadori +4

The origin of carbon-enhanced metal-poor (CEMP) stars and their possible connection with the chemical elements produced by the first stellar generation is still highly debated. In…

astro-ph.GA201477 cited

An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS), II. Discovery of Metal-poor Dusty AGB Stars

Martha L. Boyer, K. B. W. McQuinn, P. Barmby +14

The DUSTiNGS survey (DUST in Nearby Galaxies with Spitzer) is a 3.6 and 4.5 micron imaging survey of 50 nearby dwarf galaxies designed to identify dust-producing Asymptotic Giant B…

astro-ph.GA201467 cited

The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters

C. Lardo, E. Pancino, M. Bellazzini +24

The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and formation history of our Galaxy by collecting spectroscopy of representative sample…

astro-ph.GA201443 cited

13C-methyl formate: observations of a sample of high mass star-forming regions including Orion-KL and spectroscopic characterization

Cecile Favre, Miguel Carvajal, David Field +12

We have surveyed a sample of massive star-forming regions located over a range of distances from the Galactic centre for methyl formate, HCOOCH, and its isotopologues H$^{13}…

astro-ph.GA2014

AGN BLR structure, luminosity and mass from combined Reverberation Mapping and Optical Interferometry observations

Suvendu Rakshit, Romain G. Petrov

Unveiling the structure of the Broad Line Region (BLR) of AGN is critical to understand the quasar phenomenon. Detail study of the geometry and kinematic of these objects can answe…