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J. Williams

4 papers hereh-index 8169 citations15 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP2
  • astro-ph.SR2
same name
  • J. Williams — 2 papers, h 2
  • J. Williams — 2 papers, h 3
  • J. Williams — 2 papers, h 7
  • J. Williams — 2 papers, h 2
  • J. Williams — 1 paper, h 3
  • J. Williams — 1 paper, h 0

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.SR2025

ASASSN-24fw: An 8-month long, 4.1 mag, optically achromatic and polarized dimming event

R. Forés-Toribio, B. JoHantgen, C. S. Kochanek +20

We discuss ASASSN-24fw, a 13th-magnitude star that optically faded by I^”g=4.12±0.02 mag starting in September 2024 after over a decade of quiescence in ASAS-SN. The dimmimg…

astro-ph.SR2025

The accretion luminosity of Class I protostars

L. Testi, A. Natta, S. Gozzi +7

The value of the accretion luminosity during the early phases of star formation is a crucial information which helps us understand how stars form, yet it is still very difficult to…

astro-ph.EP2025

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Evidence of planet-disk interaction in the 2MASSJ16120668-3010270 system

C. Ginski, P. Pinilla, M. Benisty +28

The architectures of exoplanet systems are likely set during the initial planet-formation phase in the circumstellar disk. To understand this process, we have to study the earliest…

astro-ph.EP2025

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths

L. MatrÃ, S. Marino, D. J. Wilner +19

Planetesimal belts are ubiquitous around nearby stars, and their spatial properties hold crucial information for planetesimal and planet formation models. We present resolved dust…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.