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20042024
most citedMESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models

2.9k citations · 37.8k across the 255 of their papers we have counts for

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29 papers · 1 filter

astro-ph.GA2022★ 31 cited

Distant Echoes of the Milky Way's Last Major Merger

Vedant Chandra, Rohan P. Naidu, Charlie Conroy +9

The majority of the Milky Way's stellar halo consists of debris from our Galaxy's last major merger, the Gaia-Sausage-Enceladus (GSE). In the past few years, stars from GSE have be…

astro-ph.GA2022

What is Missing from the Local Stellar Halo?

Katherine Sharpe, Rohan P. Naidu, Charlie Conroy

The Milky Way's stellar halo, which extends to kpc, encodes the evolutionary history of our Galaxy. However, most studies of the halo to date have been limited to within a f…

astro-ph.GA2022★ 6 cited

Novae in M51: a New, Much Higher Rate from Multi-epoch HST Data

Shifra Mandel, Michael M. Shara, David Zurek +2

Accurate determination of the rates of nova eruptions in different kinds of galaxies give us strong constraints on those galaxies' underlying white dwarf and binary populations, an…

astro-ph.GA2022★ 1 cited

Dwarf galaxy archaeology from chemical abundances and star formation histories

James W. Johnson, Charlie Conroy, Benjamin D. Johnson +8

We model the stellar abundances and ages of two disrupted dwarf galaxies in the Milky Way stellar halo: Gaia-Sausage Enceladus (GSE) and Wukong/LMS-1. Using a statistically robust…

astro-ph.GA2022★ 43 cited

Rapid Quenching of Galaxies at Cosmic Noon

Minjung Park, Sirio Belli, Charlie Conroy +6

The existence of massive quiescent galaxies at high redshift seems to require rapid quenching, but it is unclear whether all quiescent galaxies have gone through this phase and wha…

astro-ph.GA2022★ 123 cited

The Poor Old Heart of the Milky Way

Hans-Walter Rix, Vedant Chandra, René Andrae +9

Massive disk galaxies like our Milky Way should host an ancient, metal-poor, and centrally concentrated stellar population. This population reflects the star formation and enrichme…

astro-ph.HE2022★ 83 cited

No peaks without valleys: The stable mass transfer channel for gravitational-wave sources in light of the neutron star-black hole mass gap

L. A. C. van Son, S. E. de Mink, M. Renzo +6

Gravitational-wave (GW) detections are starting to reveal features in the mass distribution of double compact objects. The lower end of the black hole (BH) mass distribution is esp…

astro-ph.SR2022★ 203 cited

A Sun-like star orbiting a black hole

Kareem El-Badry, Hans-Walter Rix, Eliot Quataert +18

We report discovery of a bright, nearby () Sun-like star orbiting a dark object. We identified the system as a black hole candidate via its astrometri…

astro-ph.GA2022★ 32 cited

The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history

L. A. C. van Son, S. E. de Mink, M. Chruslinska +3

New observational facilities are probing astrophysical transients such as stellar explosions and gravitational wave (GW) sources at ever increasing redshifts, while also revealing…

astro-ph.GA2022★ 2 cited

Stellar Bars in Isolated Gas-Rich Spiral Galaxies Do Not Slow Down

Angus Beane, Lars Hernquist, Elena D'Onghia +6

Elongated bar-like features are ubiquitous in galaxies, occurring at the centers of approximately two-thirds of spiral disks in the nearby Universe. Due to gravitational interactio…

astro-ph.GA2022★ 62 cited

The Stellar Halo of the Galaxy is Tilted & Doubly Broken

Jiwon Jesse Han, Charlie Conroy, Benjamin D. Johnson +7

Modern Galactic surveys have revealed an ancient merger that dominates the stellar halo of our Galaxy (\textit{Gaia}-Sausage-Enceladus, GSE). Using chemical abundances and kinemati…

astro-ph.GA2022★ 37 cited

Schrodinger's Galaxy Candidate: Puzzlingly Luminous at , or Dusty/Quenched at ?

Rohan P. Naidu, Pascal A. Oesch, David J. Setton +22

's first glimpse of the Universe has yielded a surprising abundance of luminous galaxy candidates. Here we present the most extreme of these systems: CEERS-1749. Based…

astro-ph.SR2022★ 51 cited

Magnetic braking saturates: evidence from the orbital period distribution of low-mass detached eclipsing binaries from ZTF

Kareem El-Badry, Charlie Conroy, Jim Fuller +4

We constrain the orbital period () distribution of low-mass detached main-sequence eclipsing binaries (EBs) with light curves from the Zwicky Transient Facility (ZTF),…

astro-ph.GA2022★ 6 cited

A Ghost in Boötes: The Least Luminous Disrupted Dwarf Galaxy

Vedant Chandra, Charlie Conroy, Nelson Caldwell +9

We report the discovery of Specter, a disrupted ultrafaint dwarf galaxy revealed by the H3 Spectroscopic Survey. We detected this structure via a pair of comoving metal-poor stars…

astro-ph.GA2022★ 441 cited

Two Remarkably Luminous Galaxy Candidates at Revealed by JWST

Rohan P. Naidu, Pascal A. Oesch, Pieter van Dokkum +22

The first few hundred Myrs at mark the last major uncharted epoch in the history of the Universe, where only a single galaxy (GNz11 at ) is currently spectroscop…

astro-ph.GA2022★ 29 cited

Monochromatic globular clusters as a critical test of formation models for the dark matter deficient galaxies NGC1052-DF2 and NGC1052-DF4

Pieter van Dokkum, Zili Shen, Aaron J. Romanowsky +8

It was recently proposed that the dark matter-deficient ultra-diffuse galaxies DF2 and DF4 in the NGC1052 group could be the products of a "bullet dwarf" collision between two gas-…

astro-ph.GA2022

SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass

Grecco A. Oyarzun, Kevin Bundy, Kyle B. Westfall +23

We analyze spatially resolved and co-added SDSS-IV MaNGA spectra with signal-to-noise ~100 from 2200 passive central galaxies (z~0.05) to understand how central galaxy assembly dep…

astro-ph.HE2022★ 18 cited

SRGA J181414.6-225604: A new Galactic symbiotic X-ray binary outburst triggered by an intense mass loss episode of a heavily obscured Mira variable

Kishalay De, Ilya Mereminskiy, Roberto Soria +24

We present the discovery and multi-wavelength characterization of SRGA J181414.6-225604, a Galactic hard X-ray transient discovered during the ongoing SRG/ART-XC sky survey. Using…

astro-ph.GA2022★ 97 cited

A trail of dark matter-free galaxies from a bullet dwarf collision

Pieter van Dokkum, Zili Shen, Michael A. Keim +8

The ultra-diffuse galaxies DF2 and DF4 in the NGC1052 group share several unusual properties: they both have large sizes, rich populations of overluminous and large globular cluste…

astro-ph.GA2022★ 8 cited

Live Fast, Die -Enhanced: The Mass-Metallicity- Relation of the Milky Way's Disrupted Dwarf Galaxies

Rohan P. Naidu, Charlie Conroy, Ana Bonaca +9

The Milky Way's satellite galaxies ("surviving dwarfs") have been studied for decades as unique probes of chemical evolution in the low-mass regime. Here we extend such studies to…

astro-ph.GA2022★ 29 cited

Stellar halos from The Dragonfly Edge-on Galaxies Survey

Colleen Gilhuly, Allison Merritt, Roberto Abraham +6

We present the primary results from the Dragonfly Edge-on Galaxies Survey (DEGS), an exploration of the stellar halos of twelve nearby ( Mpc) edge-on disc galaxies with the…

astro-ph.GA2022★ 38 cited

Birth of the Galactic Disk Revealed by the H3 Survey

Charlie Conroy, David H. Weinberg, Rohan P. Naidu +12

We use chemistry ([alpha/Fe] and [Fe/H]), main sequence turnoff ages, and kinematics determined from H3 Survey spectroscopy and Gaia astrometry to identify the birth of the Galacti…

astro-ph.SR2022★ 62 cited

Unicorns and Giraffes in the binary zoo: stripped giants with subgiant companions

Kareem El-Badry, Rhys Seeburger, Tharindu Jayasinghe +5

We analyze two binary systems containing giant stars, V723 Mon ("the Unicorn") and 2M04123153+6738486 ("the Giraffe"). Both giants orbit more massive but less luminous companions,…

astro-ph.GA2022★ 21 cited

A giant shell of ionized gas discovered near M82 with the Dragonfly Spectral Line Mapper pathfinder

Deborah Lokhorst, Roberto Abraham, Imad Pasha +8

We present the discovery of a giant cloud of ionized gas in the field of the starbursting galaxy M82. Emission from the cloud is seen in H and [NII]6583 in data obtained thou…