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20162026
most citedGROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR

131 citations · 1.4k across the 58 of their papers we have counts for

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Showing 2025Show all

8 papers · 1 filter

astro-ph.HE2025★ 1 cited

Revealing the accelerating wind in the inner region of the colliding-wind binary WR 112

John D. Monnier, Yinuo Han, Michael F. Corcoran +17

Colliding winds in massive binaries generate X-ray-bright shocks, synchrotron radio emission, and sometimes even dusty "pinwheel" spirals. We report the first X-ray detections of t…

astro-ph.SR2025

Constraining properties of dust formed in Wolf-Rayet binary WR 112 using mid-infrared and millimeter observations

Donglin Wu, Yinuo Han, Peredur M. Williams +9

Binaries that host a carbon-rich Wolf-Rayet (WC) star and an OB-type companion can be copious dust producers. Yet the properties of dust, particularly the grain size distribution,…

astro-ph.SR2025

A spectral library and census of near-infrared stellar large-amplitude variables from Palomar Gattini-IR

Nicholas Earley, Viraj Karambelkar, Mansi Kasliwal +9

We present a near-infrared census of stellar large-amplitude variables (LAVs) observed by the Palomar Gattini-IR (PGIR) surveyor from 2019-2021. Over the three-year time period, PG…

astro-ph.GA2025

The Sagittarius C Complex in the Mid-Infrared with SOFIA/FORCAST

Roy J. Zhao, Mark R. Morris, Matthew J. Hankins +2

We present an analysis of high-resolution mid-infrared observations at 25 and 37 of the Sagittarius C Complex (Sgr C) in the Central Molecular Zone (CMZ), based on data from t…

astro-ph.GA2025★ 1 cited

JWST interferometric imaging reveals the dusty disk obscuring the supermassive black hole of the Circinus galaxy

Enrique Lopez-Rodriguez, Joel Sanchez-Bermudez, Omaira Gonzalez-Martin +6

The dusty and molecular torus is one of the most elusive structures surrounding supermassive black holes, yet its importance is unequivocal for understanding feedback and accretion…

astro-ph.SR2025

Carbon-rich dust injected into the interstellar medium by Galactic WC binaries survives for hundreds of years

Noel D. Richardson, Micaela Henson, Emma P. Lieb +23

Some carbon-rich Wolf-Rayet stars (WC stars) show an infrared excess from dust emission. Dust forms in the collision of the WC wind with a companion star's wind. As this dust is ca…

astro-ph.SR2025★ 10 cited

Revealing a main-sequence star that consumed a planet with JWST

Ryan M. Lau, Jacob E. Jencson, Colette Salyk +8

The subluminous red nova (SLRN) ZTF SLRN-2020 is the most compelling direct detection of a planet being consumed by its host star, a scenario known as a planetary engulfment event.…

astro-ph.GA2025★ 12 cited

Dynamic Imprints of Colliding-wind Dust Formation from WR140

Emma P. Lieb, Ryan M. Lau, Jennifer L. Hoffman +24

Carbon-rich Wolf-Rayet binaries are a prominent source of carbonaceous dust that contribute to the dust budget of galaxies. The "textbook" example of an episodic dust producing WR…