activity
20062013
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 2.7k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2013★ 119 cited

Structure and evolution of high-mass stellar mergers

Evert Glebbeek, Evghenii Gaburov, Simon Portegies Zwart +1

In young dense clusters repeated collisions between massive stars may lead to the formation of a very massive star (above 100 Msun). In the past the study of the long-term evolutio…

astro-ph.HE2013★ 53 cited

Understanding Compact Object Formation and Natal Kicks. IV. The case of IC 10 X-1

Tsing-Wai Wong, Francesca Valsecchi, Asna Ansari +4

The extragalactic X-ray binary IC 10 X-1 has attracted attention as it is possibly the host of the most massive stellar-mass black-hole (BH) known to date. Here we consider all ava…

astro-ph.SR2013★ 21 cited

Mock Observations of Blue Stragglers in Globular Cluster Models

Alison Sills, Evert Glebbeek, Sourav Chatterjee +1

We created artificial color-magnitude diagrams of Monte Carlo dynamical models of globular clusters, and then used observational methods to determine the number of blue stragglers…

astro-ph.SR2013★ 71 cited

Stellar Collisions and Blue Straggler Stars in Dense Globular Clusters

Sourav Chatterjee, Frederic A. Rasio, Alison Sills +1

Blue straggler stars (BSS) are abundantly observed in all Galactic globular clusters (GGC) where data exist. However, observations alone cannot reveal the relative importance of va…

astro-ph.SR2012★ 65 cited

The Origins of Blue Stragglers and Binarity in Globular Clusters

Nathan Leigh, Christian Knigge, Alison Sills +3

(abridged) We use newly available empirical binary fractions for globular clusters to carry out a direct test of the binary evolution hypothesis, and of collisional channels that i…

astro-ph.GA2012★ 44 cited

The occurrence of nitrogen-enhanced metal-poor stars: implications for the initial mass function in the early Galactic halo

Onno R. Pols, Robert G. Izzard, Richard J. Stancliffe +1

Most carbon-enhanced metal-poor (CEMP) stars are thought to result from past mass transfer of He-burning material from an asymptotic giant branch (AGB) star to a low-mass companion…