output
20032026
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations

Showing 2023 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2023★ 92 cited

PDRs4All III: JWST's NIR spectroscopic view of the Orion Bar

Els Peeters, Emilie Habart, Olivier Berne +135

(Abridged) We investigate the impact of radiative feedback from massive stars on their natal cloud and focus on the transition from the HII region to the atomic PDR (crossing the i…

astro-ph.GA2023★ 47 cited

PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula

Emilie Habart, Els Peeters, Olivier Berné +139

The JWST has captured the most detailed and sharpest infrared images ever taken of the inner region of the Orion Nebula, the nearest massive star formation region, and a prototypic…

astro-ph.GA2023★ 11 cited

Keck Spectroscopy of NGC 1052-DF9: Stellar Populations in the Context of the NGC 1052 Group

Jonah S. Gannon, Maria Luisa Buzzo, Anna Ferré-Mateu +3

In this study, we use Keck/KCWI spectroscopy to measure the age, metallicity and recessional velocity of NGC~1052-DF9 (DF9), a dwarf galaxy in the NGC~1052 group. We compare these…

astro-ph.GA2023

Completeness of the NASA/IPAC Extragalactic Database (NED) -- Local Volume Sample

D. O. Cook, J. M. Mazzarella, G. Helou +13

We introduce the NASA/IPAC Extragalactic Database (NED) Local Volume Sample (NED-LVS), a subset of 1.9 million objects with distances out to 1000~Mpc. We use UV and IR fluxes…

astro-ph.GA2023★ 10 cited

The large-scale structure of globular clusters in the NGC 1052 group

Maria Luisa Buzzo, Duncan A. Forbes, Jean P. Brodie +4

Prompted by the many controversial claims involving the NGC 1052 group, including that it hosts two dark matter-free galaxies with overluminous and monochromatic globular cluster (…

astro-ph.GA2023★ 34 cited

A candidate runaway supermassive black hole identified by shocks and star formation in its wake

Pieter van Dokkum, Imad Pasha, Maria Luisa Buzzo +13

The interaction of a runaway supermassive black hole (SMBH) with the circumgalactic medium (CGM) can lead to the formation of a wake of shocked gas and young stars behind it. Here…