activity
20132026
most citedDoppler tomography of the circumstellar disk of π Aquarii

31 citations · 97 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

The changing optical and X-ray emission of the dormant Cas star HD 45314

G. Rauw, Y. Nazé, E. Bryssinck +25

Cas stars are Oe/Be stars that exhibit bright and hard X-ray emission. HD45314 belonged to this category, but lost its Cas characteristics as its circumstellar disc started…

astro-ph.SR2025★ 10 cited

Newborn Be star systems observed shortly after mass transfer

Th. Rivinius, R. Klement, S. D. Chojnowski +24

Many classical Be stars acquire their very rapid rotation by mass and angular-momentum transfer in massive binaries. Short-lived intermediate-phase objects have only been discovere…

astro-ph.SR2022★ 26 cited

Study of 2021 outburst of the recurrent nova RS Ophiuchi: Photoionization and morpho-kinematic modelling

Ruchi Pandey, Gesesew R. Habtie, Rahul Bandyopadhyay +3

We present the evolution of the optical spectra of the 2021 outburst of RS Ophiuchi (RS Oph) over about a month after the outburst. The spectral evolution is similar to the previou…

astro-ph.SR2020★ 1 cited

Irregular emission cycles in the Oe star HD 60848

Gregor Rauw, Yael Naze, Fran Campos +2

We analyse the spectroscopic and photometric variability of the Oe star HD 60848 over the last twenty five years. The spectra reveal recurrent, but irregular cycles of increased ci…

astro-ph.SR2019★ 9 cited

Evolution of the disk of pi Aqr: from near-disappearance to a strong maximum

Y. Naze, G. Rauw, J . Guarro Flo +30

Some Be stars display important variability of the strength of the emission lines formed in their disk. This is notably the case of pi Aqr. We present here the recent evolution of…

astro-ph.SR2018★ 20 cited

Intriguing X-ray and optical variations of the gamma Cas analog HD45314

G. Rauw, Y. Nazé, M. A. Smith +11

A growing number of Be and Oe stars, named the gamma Cas stars, are known for their unusually hard and intense X-ray emission. This emission could either trace accretion by a compa…