activity
20142022
most citedAngular Expansion of Nova Shells

24 citations · 89 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2022★ 6 cited

Planetary nebulae with Wolf-Rayet-type central stars -- IV. NGC 1501 and its mixing layer

G. Rubio, J. Toalá, H. Todt +4

Theory predicts that the temperature of the X-ray-emitting gas (10 K) detected from planetary nebulae (PNe) is a consequence of mixing or thermal conduction when in con…

astro-ph.SR2022★ 6 cited

3D mapping of the Wolf-Rayet nebula M1-67: clues for post-common envelope evolution in massive stars

S. Zavala, J. A. Toalá, E. Santamarí +5

We present a 3D mapping of the Wolf-Rayet (WR) nebula M1-67 around WR124. We obtained high-resolution San Pedro Mártir (SPM) Manchester Echelle Spectrograph (MES) observations alon…

astro-ph.SR2022★ 5 cited

Common envelope evolution in born-again planetary nebulae -- Shaping the H-deficient ejecta of A30

J. B. Rodríguez-González, E. Santamaría, J. A. Toalá +7

Born-again planetary nebulae (PNe) are extremely rare cases in the evolution of solar-like stars. It is commonly accepted that their central stars (CSPN) experienced a very late th…

astro-ph.SR2021★ 1 cited

Planetary nebulae with Wolf-Rayet-type central stars -- III. A detailed view of NGC 6905 and its central star

V. M. A. Gómez-González, G. Rubio, J. A. Toalá +6

We present a multi-wavelength characterisation of the planetary nebula (PN) NGC 6905 and its [Wolf-Rayet]-type ([WR]) central star (CSPN) HD 193949. Our Nordic Optical Telescope (N…

astro-ph.SR2021★ 2 cited

X-ray observations of the nova shell IPHASX J210204.7+471015

J. A. Toalá, G. Rubio, E. Santamaría +4

We present the analysis of XMM-Newton European Photon Imaging Camera (EPIC) observations of the nova shell IPHASX J210204.7471015. We detect X-ray emission from the progenitor b…

astro-ph.SR2020★ 11 cited

Unveiling the stellar origin of the Wolf-Rayet nebula NGC6888 through infrared observations

G. Rubio, J. A. Toalá, P. Jiménez-Hernández +5

We present a comprehensive infrared (IR) study of the iconic Wolf-Rayet (WR) wind-blown bubble NGC6888 around WR136. We use Wide-field Infrared Survey Explorer (WISE), Spitzer IRAC…