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20042026
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 10.7k across the 162 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.GA2019★ 75 cited

Metallicity and -element Abundance Gradients along the Sagittarius Stream as Seen by APOGEE

Christian R. Hayes, Steven R. Majewski, Sten Hasselquist +27

Using 3D positions and kinematics of stars relative to the Sagittarius (Sgr) orbital plane and angular momentum, we identify 166 Sgr stream members observed by the Apache Point Obs…

astro-ph.GA2019★ 177 cited

From the bulge to the outer disc: StarHorse stellar parameters, distances, and extinctions for stars in APOGEE DR16 and other spectroscopic surveys

A. B. A. Queiroz, F. Anders, C. Chiappini +27

We combine high-resolution spectroscopic data from APOGEE-2 Survey Data Release 16 (DR16) with broad-band photometric data from several sources, as well as parallaxes from {\it Gai…

astro-ph.SR2019★ 164 cited

Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview

Szabolcs Mészáros, Thomas Masseron, D. A. García-Hernández +33

We investigate the Fe, C, N, O, Mg, Al, Si, K, Ca, Ce and Nd abundances of 2283 red giant stars in 31 globular clusters from high-resolution spectra observed in both the northern a…

astro-ph.GA2019★ 95 cited

Two Ultra-Faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey

S. Mau, W. Cerny, A. B. Pace +56

We report the discovery of two ultra-faint stellar systems found in early data from the DECam Local Volume Exploration survey (DELVE). The first system, Centaurus I (DELVE J1238-40…

astro-ph.SR2019★ 86 cited

Stellar population models based on the SDSS-IV MaStar library of stellar spectra. I. Intermediate-age/old models

C. Maraston, L. Hill, D. Thomas +14

We use the first release of the SDSS/MaStar stellar library comprising ~9000, high S/N spectra, to calculate integrated spectra of stellar population models. The models extend over…

astro-ph.GA2019★ 25 cited

On the nature of a shell of young stars in the outskirts of the Small Magellanic Cloud

David Martinez-Delgado, A. Katherina Vivas, Eva K. Grebel +35

Understanding the evolutionary history of the Magellanic Clouds requires an in-depth exploration and characterization of the stellar content in their outer regions, which ultimatel…

astro-ph.GA2019

Astro2020 Science White Paper: Are Supernovae the Dust Producer in the Early Universe?

Jeonghee Rho, Danny Milisavljevic, Arkaprabha Sarangi +23

Whether supernovae are a significant source of dust has been a long-standing debate. The large quantities of dust observed in high-redshift galaxies raise a fundamental question as…

astro-ph.HE2019★ 1 cited

Achieving Transformative Understanding of Extreme Stellar Explosions with ELT-enabled Late-time Spectroscopy

D. Milisavljevic, R. Margutti, R. Chornock +35

Supernovae are among the most powerful and influential explosions in the universe. They are also ideal multi-messenger laboratories to study extreme astrophysics. However, many fun…

astro-ph.SR2019★ 122 cited

Close companions around young stars

Marina Kounkel, Kevin Covey, Maxwell Moe +26

Multiplicity is a fundamental property that is set early during stellar lifetimes, and it is a stringent probe of the physics of star formation. The distribution of close companion…

astro-ph.HE2019★ 3 cited

Multi-Messenger Astronomy with Extremely Large Telescopes

Ryan Chornock, Philip S. Cowperthwaite, Raffaella Margutti +82

The field of time-domain astrophysics has entered the era of Multi-messenger Astronomy (MMA). One key science goal for the next decade (and beyond) will be to characterize gravitat…

astro-ph.GA2019★ 123 cited

The Lazy Giants: APOGEE Abundances Reveal Low Star Formation Efficiencies in the Magellanic Clouds

David L. Nidever, Sten Hasselquist, Christian R. Hayes +28

We report the first APOGEE metallicities and alpha-element abundances measured for 3600 red giant stars spanning a large radial range of both the Large (LMC) and Small Magellanic C…