activity
20022025
most citedWASP-3b: a strongly-irradiated transiting gas-giant planet

245 citations · 539 across the 27 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2025

Near-Infrared Spectroscopy of the Recurrent Nova M31N 2008-12a

D. P. K. Banerjee, T. R. Geballe, A. Evans +3

Near infrared (NIR) 0.9--2.5m spectra of the remarkable recurrent nova M31N 2008-12a were obtained on days 6.3 and 10.3 after discovery of its 2024 outburst, and are the first N…

astro-ph.SR2025

Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays

S. Starrfield, M. Bose, C. E. Woodward +11

T Coronae Borealis (TCrB) is a recurrent nova (RN) with recorded outbursts in 1866, and 1946 and possible outbursts in 1217 and 1787. It is predicted to explode again in 2025 or 20…

astro-ph.SR2024

Near-infrared spectroscopy of the LMC recurrent nova LMCN 1968-12a

A. Evans, D. P. K. Banerjee, T. R. Geballe +5

We have obtained near-infrared (m) spectra of the recurrent nova LMCN 1968-12a on two occasions during its 2024 August eruption. This is the first near-infrared spectro…

astro-ph.SR2024

A dusty rain falls on the nova V959 Monocerotis

A. Evans, D. P. K. Banerjee, W. P. Varricatt +1

We present archival and ground-based infrared observations of the gamma-ray-emitting nova V959 Mon, covering the period 100-4205 days after the 2012 eruption. We use these data to…

astro-ph.SR2024

A Photoionization model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii

C. E. Woodward, G. Shaw, S. Starrfield +2

A near-infrared spectrum of nova V1716 Scorpii (PNV J17224490-4137160), a recent bright (V_max = 7.3 mag), Fermi-LAT detected gamma-ray source, was modeled using the photoionizatio…

astro-ph.SR2023

Snowflakes in a furnace: formation of CO and dust in a recurrent nova eruption

D. P. K. Banerjee, C. E. Woodward, V. Joshi +7

We report the detection of carbon monoxide (CO) and dust, formed under hostile conditions, in recurrent nova V745 Sco about 8.7 days after its 2014 outburst. The formation of molec…