activity
20022019
most citedStudies of Variability in Proto-Planetary Nebulae: II. Light and Velocity Curve Analyses of Iras 22272+5435 and 22223+4327

30 citations · 174 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2019★ 28 cited

The compact multiple system HIP 41431

T. Borkovits, J. Sperauskas, A. Tokovinin +4

The nearby (50 pc) K7V dwarf HIP~41431 (EPIC 212096658) is a compact 3-tier hierarchy. Three K7V stars with similar masses, from 0.61 to 0.63 solar, make a triple-lined spectroscop…

astro-ph.SR2019★ 29 cited

Spectroscopic orbits of nearby stars

J. Sperauskas, V. Deveikis, A. Tokovinin

We observed stars with variable radial velocities to determine their spectroscopic orbits. Velocities of 132 targets taken over a time span reaching 30 years are presented. They we…

astro-ph.SR2018★ 1 cited

Variability in Proto-Planetary Nebulae: V. Velocity and Light Curve Analyses of IRAS 17436+5003, 18095+2704, and 19475+3119

Bruce J. Hrivnak, Griet Van de Steene, Hans Van Winckel +2

We have obtained contemporaneous light, color, and radial velocity data for three proto-planetary nebulae (PPNe) over the years 2007 to 2015. The light and velocity curves of each…

astro-ph.SR2017★ 27 cited

Where Are the Binaries? Results of a Long-Term Search for Radial Velocity Binaries in Proto-Planetary Nebulae

Bruce J. Hrivnak, Griet Van de Steene, Hans Van Winckel +3

We present the results of an expanded, long-term radial velocity search (25 yrs) for evidence of binarity in a sample of seven bright proto-planetary nebulae (PPNe). The goal is to…

astro-ph.SR2015★ 19 cited

Spectroscopic variability of IRAS22272+5435

L. Začs, F. Musaev, B. Kaminsky +4

A time series of high-resolution spectra was observed in the optical wavelength region for the bright proto-planetary nebula IRAS22272+5435 (HD235858), along with a simultaneous mo…

astro-ph.IM2013

A new empirical metallicity calibration for Vilnius photometry

S. Bartasiute, S. Raudeliunas, J. Sperauskas

We present a new calibration of the seven-color Vilnius system in terms of [Fe/H], applicable to F-M stars in the metallicity range -2.8<[Fe/H]<+0.5. We employ a purely empirical a…