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20132023
most citedIlluminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger

822 citations · 2k across the 48 of their papers we have counts for

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21 papers · 1 filter

astro-ph.SR2023

FORCASTing the spectroscopic dust properties of the WC+O binary WR137 with SOFIA

Megan J. Peatt, Noel D. Richardson, Peredur M. Williams +5

WR 137 (HD 192641) is a binary system consisting of a carbon-rich Wolf-Rayet star and an Oe companion star in a 13-year orbit. Near periastron, the winds of the two stars collide a…

astro-ph.SR2023★ 83 cited

A Luminous Red Supergiant and Dusty Long-period Variable Progenitor for SN 2023ixf

Jacob E. Jencson, Jeniveve Pearson, Emma R. Beasor +23

We analyze pre-explosion near- and mid-infrared (IR) imaging of the site of SN 2023ixf in the nearby spiral galaxy M101 and characterize the candidate progenitor star. The star dis…

astro-ph.SR2023★ 10 cited

From Dust to Nanodust: Resolving Circumstellar Dust from the Colliding-Wind Binary Wolf-Rayet (WR) 140

Ryan M. Lau, Jason Wang, Matthew J. Hankins +17

Wolf-Rayet (WR) 140 is the archetypal periodic dust-forming colliding-wind binary that hosts a carbon-rich WR (WC) star and an O-star companion with an orbital period of 7.93 years…

astro-ph.SR2022

Recurring outbursts of the supernova impostor AT 2016blu in NGC 4559

Mojgan Aghakhanloo, Nathan Smith, Peter Milne +8

We present the first photometric analysis of the supernova (SN) impostor AT 2016blu in NGC 4559. This transient was discovered by the Lick Observatory Supernova Search in 2012 and…

astro-ph.SR2022★ 21 cited

Radiation-driven acceleration in the expanding WR140 dust shell

Yinuo Han, Peter G. Tuthill, Ryan M. Lau +1

The Wolf-Rayet (WR) binary system WR140 is a close (0.9-16.7 mas) binary star consisting of an O5 primary and WC7 companion and is known as the archetype of episodic dust-producing…

astro-ph.SR2022★ 60 cited

Nested Dust Shells around the Wolf-Rayet Binary WR 140 observed with JWST

Ryan M. Lau, Matthew J. Hankins, Yinuo Han +29

Massive colliding-wind binaries that host a Wolf-Rayet (WR) star present a potentially important source of dust and chemical enrichment in the interstellar medium (ISM). However, t…

astro-ph.SR2022

Detection of a broad 8 m UIR feature in the mid-infrared spectrum of WR 125 observed with Subaru/COMICS

Izumi Endo, Ryan M. Lau, Itsuki Sakon +3

We present the detection of a broad 8 m feature in newly formed dust around the carbon-rich Wolf-Rayet (WC) binary WR 125 from N-band low-resolution (NL; R250) spectroscop…

astro-ph.SR2021★ 1 cited

Discovery of a 310-day Period from the Enshrouded Massive System NaSt1 (WR 122)

Ryan M. Lau, Samaporn Tinyanont, Matthew J. Hankins +15

We present optical and infrared (IR) light curves of NaSt1, also known as Wolf-Rayet (WR) 122, with observations from Palomar Gattini-IR (PGIR), the Zwicky Transient Facility (ZTF)…

astro-ph.SR2021★ 16 cited

Outbursting Young Stellar Object PGIR 20dci in the Perseus Arm

Lynne A. Hillenbrand, Kishalay De, Matthew Hankins +9

We report the discovery of a likely outbursting Class I young stellar object, associated with the star-forming region NGC 281-W (distance kpc). The source is currently s…

astro-ph.SR2021

AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary

Jacob E. Jencson, Jennifer E. Andrews, Howard E. Bond +39

Nova eruptions, thermonuclear explosions on the surfaces of white dwarfs (WDs), are now recognized to be among the most common shock-powered astrophysical transients. We present th…

astro-ph.SR2021★ 5 cited

The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor

Nadejda Blagorodnova, Jakub Klencki, Ondrej Pejcha +12

Luminous Red Novae (LRNe) are astrophysical transients associated with the partial ejection of a binary system's common envelope (CE) shortly before its merger. Here we present the…

astro-ph.SR2020★ 18 cited

Census of R Coronae Borealis stars I: Infrared light curves from Palomar Gattini IR

Viraj R. Karambelkar, Mansi M. Kasliwal, Patrick Tisserand +16

We are undertaking the first systematic infrared (IR) census of R Coronae Borealis (RCB) stars in the Milky Way, beginning with IR light curves from the Palomar Gattini IR (PGIR) s…

astro-ph.SR2020★ 19 cited

The extreme colliding-wind system Apep: resolved imagery of the central binary and dust plume in the infrared

Y. Han, P. G. Tuthill, R. M. Lau +6

The recent discovery of a spectacular dust plume in the system 2XMM J160050.7-514245 (referred to as "Apep") suggested a physical origin in a colliding-wind binary by way of the "P…

astro-ph.SR2020

Resolving Decades of Periodic Spirals from the Wolf-Rayet Dust Factory WR 112

Ryan M. Lau, Matthew J. Hankins, Yinuo Han +9

WR 112 is a dust-forming carbon-rich Wolf-Rayet (WC) binary with a dusty circumstellar nebula that exhibits a complex asymmetric morphology, which traces the orbital motion and dus…

astro-ph.SR2020★ 40 cited

Revisiting the Impact of Dust Production from Carbon-Rich Wolf-Rayet Binaries

Ryan M. Lau, J. J. Eldridge, Matthew J. Hankins +3

We present a dust spectral energy distribution (SED) and binary stellar population analysis revisiting the dust production rates (DPRs) in the winds of carbon-rich Wolf-Rayet (WC)…

astro-ph.SR2019★ 30 cited

Supernova 2014C: ongoing interaction with extended circumstellar material with silicate dust

Samaporn Tinyanont, Ryan M Lau, Mansi M Kasliwal +8

Supernova (SN) 2014C is a unique explosion where a seemingly typical hydrogen-poor stripped envelope SN started to interact with a dense, hydrogen-rich circumstellar medium (CSM) a…

astro-ph.SR2019★ 31 cited

Discovery of an intermediate-luminosity red transient in M51 and its likely dust-obscured, infrared-variable progenitor

Jacob E. Jencson, Scott M. Adams, Howard E. Bond +49

We present the discovery of an optical transient (OT) in Messier 51, designated M51 OT2019-1 (also ZTF19aadyppr, AT 2019abn, ATLAS19bzl), by the Zwicky Transient Facility (ZTF). Th…

astro-ph.SR2017★ 3 cited

An Optical and Infrared Time-Domain Study of the Supergiant Fast X-ray Transient Candidate IC 10 X-2

Stephanie Kwan, Ryan M. Lau, Jacob Jencson +5

We present an optical and infrared (IR) study of IC 10 X-2, a high-mass X-ray binary in the galaxy IC 10. Previous optical and X-ray studies suggest X-2 is a Supergiant Fast X-ray…

astro-ph.SR2016★ 11 cited

Stagnant Shells in the Vicinity of the Dusty Wolf-Rayet-OB Binary WR 112

R. M. Lau, M. J. Hankins, R. Schödel +3

We present high spatial resolution mid-infrared images of the nebula around the late-type carbon-rich Wolf-Rayet (WC)-OB binary system WR~112 taken by the recently upgraded VLT spe…

astro-ph.SR2016★ 62 cited

A Systematic Study of Mid-Infrared Emission from Core-Collapse Supernovae with SPIRITS

Samaporn Tinyanont, Mansi M. Kasliwal, Ori D. Fox +12

We present a systematic study of mid-infrared (mid-IR) emission from 141 nearby supernovae (SNe) observed with the InfraRed Array Camera (IRAC) on Spitzer.These SNe reside in one o…

astro-ph.SR2015

SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment

J. D. Adams, T. L. Herter, J. L. Hora +22

We present mid-IR (19 - 37 microns) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6 - 8.0 microns), IRTF/MIRLIN (11.3 and…