activity
20062023
most citedCarnegie Supernova Project-II: The Near-infrared Spectroscopy Program

87 citations · 374 across the 18 of their papers we have counts for

collaborators

19 papers

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…

astro-ph.SR2023★ 8 cited

V445 Puppis -- Dustier than a Thousand Novae

D. P. K. Banerjee, A. Evans, C. E. Woodward +4

V445 Puppis, the only known Galactic helium nova, is a unique test-bed to verify supernova (SN) theories in the single degenerate channel that involve a white dwarf (WD) accreting…

astro-ph.SR2023★ 11 cited

Infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco

A. Evans, D. P. K. Banerjee, C. E. Woodward +5

We present near-infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco, over the period from 5.2 to 45.4 days after outburst. This is the most intensive infrared st…

astro-ph.SR2022★ 10 cited

Infrared spectroscopy of the 2019 eruption of the recurrent nova V3890 Sgr: separation into equatorial and polar winds revealed

A. Evans, T. R. Geballe, C. E. Woodward +4

We present infrared spectroscopy of the 2019 eruption of the recurrent nova V3890 Sgr, obtained over the period 5.1-46.3 days after the eruption. The spectrum of the red giant beca…

astro-ph.SR2022

Stringent limits on SiO maser emission from the recurrent nova T Coronae Borealis

A. Evans, B. Pimpanuwat, A. M. S. Richards +5

There are indications that the third known eruption of the recurrent nova T CrB is imminent, and multi-wavelength observations prior to the eruption are important to characterise t…

astro-ph.SR2022★ 3 cited

The recurrent nova V3890~Sgr: a near-infrared and optical study of the red giant component and its environment

B. Kaminsky, A. Evans, Ya. V. Pavlenko +8

We present an analysis of the red giant component of the recurrent nova V3890 Sgr, using data obtained before and after its 2019 eruption. Its effective temperature is $T_{\rm eff}…