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19962023
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 42.3k across the 239 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA2019★ 33 cited

Stars made in outflows may populate the stellar halo of the Milky Way

Sijie Yu, James S. Bullock, Andrew Wetzel +8

We study stellar-halo formation using six Milky Way-mass galaxies in FIRE-2 cosmological zoom simulations. We find that of the outer ( kpc) stellar halo in each sy…

astro-ph.GA2019★ 51 cited

Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM

Saundra M. Albers, Daniel R. Weisz, Andrew A. Cole +11

We present the star formation history (SFH) of the isolated (D~970 kpc) Local Group dwarf galaxy WLM measured from color-magnitude diagrams constructed from deep Hubble Space Teles…

astro-ph.GA2019★ 45 cited

The Halos and Environments of Nearby Galaxies (HERON) I: Imaging, Sample Characteristics, and Envelope Diameters

R. Michael Rich, Aleksandr Mosenkov, Henry Lee-Saunders +16

We use a dedicated 0.7-m telescope to image the halos of 119 galaxies in the Local Volume to mag/arcsec. The sample is primarily from the 2MASS Large Galaxy At…

astro-ph.GA2019★ 13 cited

Accurate mass estimates from the proper motions of dispersion-supported galaxies

Alexandres Lazar, James S. Bullock

Starting with the spherical Jeans equation, we show that there exists a radius where the mass enclosed depends only on the projected tangential velocity dispersion, assuming that t…

astro-ph.GA2019★ 33 cited

Characterizing the Infall Times and Quenching Timescales of Milky Way Satellites with Proper Motions

Sean P. Fillingham, Michael C. Cooper, Tyler Kelley +6

Observations of low-mass satellite galaxies in the nearby Universe point towards a strong dichotomy in their star-forming properties relative to systems with similar mass in the fi…

astro-ph.GA2019★ 129 cited

A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations

Jenna Samuel, Andrew Wetzel, Erik Tollerud +9

While many tensions between Local Group (LG) satellite galaxies and LCDM cosmology have been alleviated through recent cosmological simulations, the spatial distribution of satelli…

astro-ph.GA2019★ 135 cited

Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment

Shea Garrison-Kimmel, Andrew Wetzel, Phillip F. Hopkins +13

We study star formation histories (SFHs) of dwarf galaxies (stellar mass ) from FIRE-2 cosmological zoom-in simulations. We compare dwarf…

astro-ph.GA2019★ 24 cited

Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?

Marcel S. Pawlowski, James S. Bullock, Tyler Kelley +1

The Milky Way, the Andromeda galaxy, and Centaurus A host flattened distributions of satellite galaxies which exhibits coherent velocity trends indicative of rotation. Comparably e…

astro-ph.GA2019★ 6 cited

Understanding the circumgalactic medium is critical for understanding galaxy evolution

Molly S. Peeples, Peter Behroozi, Rongmon Bordoloi +69

Galaxies evolve under the influence of gas flows between their interstellar medium and their surrounding gaseous halos known as the circumgalactic medium (CGM). The CGM is a major…

astro-ph.GA2019★ 66 cited

The Milky Way's Halo and Subhalos in Self-Interacting Dark Matter

Victor H. Robles, Tyler Kelley, James S. Bullock +1

We perform high-resolution simulations of a MW-like galaxy in a self-interacting cold dark matter model with elastic cross section over mass of (SIDM) and compare to…

astro-ph.GA2019★ 43 cited

A Predicted Correlation Between Age Gradient and Star Formation History in FIRE Dwarf Galaxies

Andrew S. Graus, James S. Bullock, Alex Fitts +9

We explore the radial variation of star formation histories in dwarf galaxies simulated with Feedback In Realistic Environments (FIRE) physics. The sample contains 9 low-mass field…