activity
19972026
most citedVVV DR1: The First Data Release of the Milky Way Bulge and Southern Plane from the Near-Infrared ESO Public Survey VISTA Variables in the Via Lactea

409 citations · 3.9k across the 61 of their papers we have counts for

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Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2024★ 8 cited

Spectroscopic observations of flares and superflares on AU Mic

P. Odert, M. Leitzinger, R. Greimel +13

The young active flare star AU~Mic is the planet host star with the highest flare rate from TESS data. Therefore, it represents an ideal target for dedicated ground-based monitorin…

astro-ph.SR2023

Mass ratio of single-line spectroscopic binaries with visual orbits using Bayesian inference and suitable priors

Jennifer Anguita-Aguero, Rene A. Mendez, Miguel Videla +4

We present orbital elements for twenty-two single-line binaries, nine of them studied for the first time, determined from a joint spectroscopic and astrometric solution. The astrom…

astro-ph.SR2019★ 10 cited

A new look into putative duplicity and pulsations of the Be star CMi

P. Harmanec, M. Svanda, D. Korcakova +6

Bright Be star beta CMi has been identified as a non-radial pulsator on the basis of space photometry with the MOST satellite and also as a single-line spectroscopic binary with a…

astro-ph.SR2018★ 30 cited

Beryllium detection in the very fast nova ASASSN-16kt (V407 Lupi)

L. Izzo, P. Molaro, P. Bonifacio +8

We present high-resolution spectroscopic observations of the fast nova ASASSN-16kt (V407 Lup). A close inspection of spectra obtained at early stages has revealed the presence of l…

astro-ph.SR2018

Ori and Lib: Two new massive heartbeat binaries

Andrzej Pigulski, Monika K. Kaminska, Krzysztof Kaminski +28

We report the discovery of two massive eccentric systems with BRITE data, Ori and Lib, showing heartbeat effects close to the periastron passage. Lib exhibits shallow e…

astro-ph.SR2017★ 37 cited

Stellar parameters and H line profile variability of Be stars in the BeSOS survey

C. Arcos, S. Kanaan, J. Chávez +3

The Be phenomenon is present in about 20 of the B-type stars. Be stars show variability on a broad range of timescales, which in most cases is related to the presence of a circ…