A dusty rain falls on the nova V959 Monocerotis

Evans, A; Banerjee, D P K; Varricatt, W P; Joshi, V

doi:10.1093/mnras/stae1240

All Outputs (2)

A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii (2024)
Journal Article
Woodward, C. E., Shaw, G., Starrfield, S., Evans, A., & Page, K. L. (2024). A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii. Astrophysical Journal, 968(1), Article 31. https://doi.org/10.3847/1538-4357/ad4097

A near-infrared spectrum of nova V1716 Scorpii (PNV J17224490-4137160), a recent bright ( Vmax=7.3 mag), Fermi-LAT detected γ-ray source, was modeled using the photoionization code CLOUDY. Abundances were estimated for He, C, N, O, Si, Al, Mg, Fe, Ne... Read More about A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii.

A dusty rain falls on the nova V959 Monocerotis (2024)
Journal Article
Evans, A., Banerjee, D. P. K., Varricatt, W. P., & Joshi, V. (2024). A dusty rain falls on the nova V959 Monocerotis. Monthly Notices of the Royal Astronomical Society, 531(1), 728-738. https://doi.org/10.1093/mnras/stae1240

We present archival and ground-based infrared observations of the γ-ray-emitting nova V959 Mon, covering the period 100–4205 d after the 2012 eruption. We use these data to determine that the secondary in the nova system is a G5 main sequence star. D... Read More about A dusty rain falls on the nova V959 Monocerotis.