output
20012026
most citedFluxes in Hαand Ca II H and K for a sample of Southern stars

180 citations

Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

A very rapidly rotating white dwarf in nova YZ Reticuli

G. J. M. Luna, N. Rawat, R. Angeloni +4

YZ Ret (Nova Reticuli 2020) is the first VY Scl-type nova-like variable observed to undergo a classical nova eruption. Following the outburst, timing analysis of 20-s cadence TESS…

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

A TESS View of Post-Eruption Variability in the Novae V1405 Cas,V1716 Sco, and V1674 Her

G. J. M. Luna, A. Dobrotka, M. Orio

We analyzed TESS archival data of three novae after recent outbursts, searching the orbital and white dwarf (WD) rotation period and possible variations of these periods. In V1405…

astro-ph.SR2021★ 20 cited

Searching for new solar twins: The Inti survey for the Northern Sky

J. Y. Galarza, R. López-Valdivia, D. Lorenzo-Oliveira +9

Solar twins are key in different areas of astrophysics, however only just over a hundred were identified and well-studied in the last two decades. In this work, we take advantage o…

astro-ph.SR2014★ 20 cited

Discovery of a new PG1159 (GW Vir) Pulsator

S. O. Kepler, Luciano Fraga, Don Earl Winget +3

We report the discovery of pulsations in the spectroscopic PG 1159 type pre-white dwarf SDSS J075415.12+085232.18. Analysis of the spectrum by Werner, Rauch and Kepler (2014) indic…

astro-ph.SR2014★ 66 cited

On the incidence of eclipsing Am binary systems in the SuperWASP survey

B. Smalley, J. Southworth, O. I. Pintado +18

The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analyse…