activity
19972026
most citedIlluminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger

822 citations · 11.7k across the 195 of their papers we have counts for

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42 papers · 1 filter

astro-ph.SR2026

The FU Ori outburst of PR Ori B

Carlos Contreras Pena, Zsofia Nagy, Gregory Herczeg +42

We report the discovery of a nearby FU Ori-type outburst (FUor), PR Ori B, in the L1641 cluster of the Orion star-forming region. The high-amplitude variability was first identifie…

astro-ph.SR2023★ 12 cited

The HH 24 Complex: Jets, Multiple Star Formation, and Orphaned Protostars

Bo Reipurth, J. Bally, Hsi-Wei Yen +9

The HH 24 complex harbors five collimated jets emanating from a small protostellar multiple system. We have carried out a multi-wavelength study of the jets, their driving sources,…

astro-ph.SR2022★ 11 cited

Dents in the Veil: Protostellar feedback in Orion

U. Kavak, J. Bally, J. R. Goicoechea +3

Interest in stellar feedback has recently increased because new studies suggest that radiative and mechanical feedback from young massive stars regulate the physical and chemical c…

astro-ph.SR2022★ 2 cited

Hubble Space Telescope Imaging of Luminous Extragalactic Infrared Transients and Variables from the SPIRITS Survey

Howard E. Bond, Jacob E. Jencson, Patricia A. Whitelock +6

SPIRITS--the SPitzer InfraRed Intensive Transients Survey--searched for luminous infrared (IR) transients and variables in nearly 200 nearby galaxies from 2014 to 2019, using the w…

astro-ph.SR2020★ 7 cited

Accretion and outflow activity in proto-brown dwarfs

B. Riaz, J. Bally

We present a near-infrared study of accretion and outflow activity in 6 Class 0/I proto-brown dwarfs (proto-BDs) using VLT/SINFONI spectroscopy and spectro-imaging observations. Th…

astro-ph.SR2020★ 12 cited

Star Cluster Formation in Orion A

Wanggi Lim, Fumitaka Nakamura, Benjamin Wu +9

We introduce new analysis methods for studying the star cluster formation processes in Orion A, especially examining the scenario of a cloud-cloud collision. We utilize the CARMA-N…