activity
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

collaborators
Showing 2024 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2024

Discovery and Spectroscopic Confirmation of Aquarius III: A Low-Mass Milky Way Satellite Galaxy

W. Cerny, A. Chiti, M. Geha +37

We present the discovery of Aquarius III, an ultra-faint Milky Way satellite galaxy identified in the second data release of the DECam Local Volume Exploration (DELVE) survey. Base…

astro-ph.GA2024★ 19 cited

A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Galaxy with DELVE Early Data Release 3

C. Y. Tan, W. Cerny, A. Drlica-Wagner +32

We report the discovery and spectroscopic confirmation of an ultra-faint Milky Way (MW) satellite in the constellation of Leo. This system was discovered as a spatial overdensity o…

astro-ph.GA2024

Unveiling the purely young star formation history of the SMC's northeastern shell from colour-magnitude diagram fitting

Joanna D. Sakowska, Noelia E. D. Noël, Tomás Ruiz-Lara +12

We obtain a quantitative star formation history (SFH) of a shell-like structure ('shell') located in the northeastern part of the Small Magellanic Cloud (SMC). We use the Survey of…

astro-ph.GA2024★ 2 cited

The SDSS-V Local Volume Mapper (LVM): Scientific Motivation and Project Overview

Niv Drory, Guillermo A. Blanc, Kathryn Kreckel +48

We present the Sloan Digital Sky Survey V (SDSS-V) Local Volume Mapper (LVM). The LVM is an integral-field spectroscopic survey of the Milky Way, Magellanic Clouds, and of a sample…

astro-ph.GA2024★ 24 cited

SDSS-V Local Volume Mapper (LVM): A Glimpse into Orion

K. Kreckel, O. V. Egorov, E. Egorova +37

The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedb…

astro-ph.GA2024★ 2 cited

Carbon- and Oxygen-rich stars in MaStar: identification and classification

Lewis Hill, Claudia Maraston, Daniel Thomas +5

Carbon- and Oxygen-rich stars populating the Thermally-Pulsing Asymptotic Giant Branch (TP-AGB) phase of stellar evolution are relevant contributors to the spectra of ~1 Gyr old po…

astro-ph.GA2024

A perspective on the Milky Way Bulge-Bar as seen from the neutron-capture elements Cerium and Neodymium with APOGEE

J. V. Sales-Silva, K. Cunha, V. V. Smith +28

This study probes the chemical abundances of the neutron-capture elements cerium and neodymium in the inner Milky Way from an analysis of a sample of 2000 stars in the Galact…