activity
20202026
most citedChandra High Energy Transmission Gratings Spectra of V3890 Sgr

27 citations · 33 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

A micronova burst in the intermediate polar IGR J17014-4306

Alexandre S. Oliveira, D. C. Souza, G. J. M. Luna +1

We report the detection of a short optical burst in TESS data of IGR J17014-4306, the eclipsing intermediate polar with the longest known orbital period. The burst lasts 1.56 d and…

astro-ph.SR2026

The accretion-driven eruption of the recurrent nova T Corona Borealis

Raymundo Baptista, Wagner Schlindwein, Gerardo J. M. Luna

T Corona Borealis (T CrB) is a symbiotic recurrent nova with an yr recurrence interval, the eruptions of which occur on top of a yr long high-brightness sta…

astro-ph.SR2026★ 1 cited

A search for new symbiotic stars in the Milky Way: Using machine learning techniques applied to photometric databases

V. Contreras Rojas, M. Jaque Arancibia, C. E. Ferreira Lopes +8

Symbiotic stars (SySts) are interacting binaries composed of a red giant transferring material to a hot compact star, typically a white dwarf. Although only about 300 systems are c…

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.HE2025★ 4 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★ 1 cited

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.HE2024

V407 Lup, an intermediate polar nova

M. Orio, M. Melicherčík, S. Ciroi +6

We present X-ray and optical observations of nova V407 Lup (Nova Lup 2016), previously well monitored in outburst, as it returned to quiescent accretion. The X-ray light curve in 2…

astro-ph.HE2020★ 27 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…