output
19952026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2018 · astro-ph.SRShow all

6 papers · 2 filters

astro-ph.SR2018★ 5 cited

The collisional atomic processes of Rydberg alkali atoms in Geo-cosmical plasmas

Lj. M. Ignjatovic, V. A. Sreckovic, M. S. Dimitrijevic

The chemi-ionization (CI) processes in atom-Rydberg-atom collisions are investigated in this contribution. The rate coefficients for CI processes in $\textrm{Li}^{*}(n) + \textrm{N…

astro-ph.SR2018★ 7 cited

Differential interferometry of the rapid rotator Regulus

M. Hadjara, R. G. Petrov, S. Jankov +3

We analyse interferometric data obtained for Regulus with AMBER (Astronomical Multi- BEam combineR) at high spectral resolution () across the Br spectral line…

astro-ph.SR2018★ 2 cited

OGLE-2014-BLG-0962 and the First Statistical Validation of Bayesian Priors for Galactic Microlensing

Yutong Shan, Jennifer C. Yee, Andrzej Udalski +46

OGLE-2014-BLG-0962 (OB140962) is a stellar binary microlensing event that was well-covered by observations from the Spitzer satellite as well as ground-based surveys. Modelling yie…

astro-ph.SR2018

Shockwave Behaviour in RR Lyrae Stars

Attila Bódi, László Molnár, Emese Plachy +1

Here we present the detailed analysis of some modulated Kepler and K2 RR Lyrae stars that show peculiar bump progression in respect to the pulsation phase.

astro-ph.SR2018★ 18 cited

Structural changes in the hot Algol OGLE-LMC-DPV-097 and its disk related to its long-cycle

J. Garcés L., R. E. Mennickent, G. Djurasević +2

Double Periodic Variables (DPVs) are hot Algols showing a long photometric cycle of uncertain origin. We report the discovery of changes in the orbital light curve of OGLE-LMC-DPV-…

astro-ph.SR2018★ 17 cited

Spectroscopic and photometric study of the eclipsing interacting binary V495 Centauri

J. A. Rosales, R. E. Mennickent, G. Djurašević +2

Double Periodic Variables (DPV) are among the new enigmas of semi-detached eclipsing binaries. These are intermediate-mass binaries characterized by a long photometric period lasti…