activity
20202025
most citedChandra High Energy Transmission Gratings Spectra of V3890 Sgr

27 citations · 31 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

No evidence of intrinsic linear polarization in Nova Vel 2025 (V572 Vel)

Isabel J. Lima, Marina M. C. Mello, Claudia V. Rodrigues +3

We report on polarimetric observations of V572 Vel (Nova Vel 2025) conducted on June 26th and July 21st, 2025, shortly after its nova eruption was discovered. Our measurements in t…

astro-ph.HE20254 cited

Broad Observational Perspectives Achieved by the Accreting White Dwarf Sciences in the XMM-Newton and Chandra Eras

Solen Balman, Marina Orio, Gerardo J. M. Luna

Accreting white dwarf binaries (AWDs) comprise cataclysmic variables (CVs), symbiotics, AM CVns, and other related systems that host a primary white dwarf (WD) accreting from a mai…

astro-ph.SR2025

Detection of the white-dwarf spin of V1082 Sgr

I. J. Lima, G. Tovmassian, C. V. Rodrigues +9

We report on the discovery of circular polarization modulated with a period of 1.943 +- 0.002 h in the cataclysmic variable V1082 Sgr. These findings unambiguously reveal the rotat…

astro-ph.EP2025

The EXO-UV program: lastest advances of experimental studies to investigate the biological impact of UV radiation on exoplanets

Ximena C. Abrevaya, Petra Odert, Oscar J. Oppezzo +4

The EXO-UV program is an international, interdisciplinary collaboration between astrophysicists and biologists aimed at expanding the characterization of ultraviolet radiation (UVR…

astro-ph.SR2024

A new way to find symbiotic stars: accretion disc detection with continuum survey photometry

A. B. Lucy, J. L. Sokoloski, G. J. M. Luna +10

Symbiotic stars are binaries in which a cool and evolved star of luminosity class I-III accretes onto a smaller companion. However, direct accretion signatures like disc flickering…

astro-ph.HE202027 cited

Chandra High Energy Transmission Gratings Spectra of V3890 Sgr

Marina Orio, Jeremy J. Drake, Jan-Uwe Ness +13

The recurrent nova (RN) V3890 Sgr was observed during the 7th day after the onset of its most recent outburst, with the Chandra ACIS-S camera and High Energy Transmission Gratings…