activity
20002019
most citedStellar Feedback in Dwarf Galaxy Formation

376 citations · 1.1k across the 16 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2019★ 70 cited

Modeling the light curve of `Oumuamua: evidence for torque and disc-like shape

Sergey Mashchenko

We present the first attempt to fit the light curve of the interstellar visitor `Oumuamua using a physical model which includes optional torque. We consider both conventional (Lomm…

astro-ph.GA2015★ 4 cited

Mass Models of Dwarf Spheroidal Galaxies with Variable Stellar Anisotropy. I. Jeans Analysis

Sergey Mashchenko

Using a flexible galactic model with variable stellar velocity anisotropy, I apply the classical Jeans mass modeling approach to the five dwarf spheroidal galaxies with the largest…

astro-ph.GA2012★ 22 cited

Building the Stellar Halo Through Feedback in Dwarf Galaxies

Aaron J. Maxwell, James Wadsley, H. M. P. Couchman +1

We present a new model for the formation of stellar halos in dwarf galaxies. We demonstrate that the stars and star clusters that form naturally in the inner regions of dwarfs are…

astro-ph2007★ 376 cited

Stellar Feedback in Dwarf Galaxy Formation

Sergey Mashchenko, James Wadsley, H. M. P. Couchman

Dwarf galaxies pose significant challenges for cosmological models. In particular, current models predict a dark matter density that is divergent at the center, in sharp contrast w…

astro-ph2006★ 295 cited

Cosmological puzzle resolved by stellar feedback in high redshift galaxies

Sergey Mashchenko, H. M. P. Couchman, James Wadsley

The standard cosmological model, now strongly constrained by direct observation at early epochs, is very successful in describing the structure of the evolved universe on large and…

astro-ph2005★ 35 cited

Constraining global properties of the Draco dwarf spheroidal galaxy

Sergey Mashchenko, Alison Sills, H. M. P. Couchman

By fitting a flexible stellar anisotropy model to the observed surface brightness and line-of-sight velocity dispersion profiles of Draco we derive a sequence of cosmologically pla…