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19962026
most citedHigher Charmonia

809 citations · 28.2k across the 927 of their papers we have counts for

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Showing 2018 · astro-ph.SRShow all

10 papers · 2 filters

astro-ph.SR2018★ 31 cited

New Near-Infrared light-curve templates for RR Lyrae variables

V. F. Braga, P. B. Stetson, G. Bono +34

We provide homogeneous optical (UBVRI) and near-infrared (JHK) time series photometry for 254 cluster (omega Cen, M4) and field RR Lyrae (RRL) variables. We ended up with more than…

astro-ph.SR2018★ 54 cited

Burst occurrence in young massive stellar objects

Meyer D. M. -A., Vorobyov E. I., Elbakyan V. G. +3

Episodic accretion-driven outbursts are an extreme manifestation of accretion variability. It has been proposed that the development of gravitational instabilities in the proto-cir…

astro-ph.SR2018★ 21 cited

Solar flares and Kelvin-Helmholtz instabilities: A parameter survey

Wenzhi Ruan, Chun Xia, Rony Keppens

Hard X-ray (HXR) sources are frequently observed near the top of solar flare loops, and the emission is widely ascribed to bremsstrahlung. We here revisit an alternative scenario w…

astro-ph.SR2018★ 37 cited

Explosions of blue supergiants from binary mergers for SN 1987A

Athira Menon, Victor Utrobin, Alexander Heger

Based on the work of Menon & Heger (2017), we present the bolometric light curvesand spectra of the explosions of blue supergiant progenitors from binary mergers. We study SN 1987A…

astro-ph.SR2018★ 25 cited

An investigation of the photometric variability of confirmed and candidate Galactic Be stars using ASAS-3 data

Klaus Bernhard, Sebastián Otero, Stefan Hümmerich +3

We present an investigation of a large sample of confirmed (N=233) and candidate (N=54) Galactic classical Be stars (mean V magnitude range of 6.4 to 12.6 mag), with the main aim o…

astro-ph.SR2018★ 10 cited

New Cepheid variables in the young open clusters Berkeley 51 and Berkeley 55

M. E. Lohr, I. Negueruela, H. M. Tabernero +3

As part of a wider investigation of evolved massive stars in Galactic open clusters, we have spectroscopically identified three candidate classical Cepheids in the little-studied c…

astro-ph.SR2018★ 33 cited

The Arches cluster revisited: II. A massive eclipsing spectroscopic binary in the Arches cluster

M. E. Lohr, J. S. Clark, F. Najarro +3

We have carried out a spectroscopic variability survey of some of the most massive stars in the Arches cluster, using K-band observations obtained with SINFONI on the VLT. One targ…

astro-ph.SR2018★ 69 cited

Accelerating infall and rotational spin-up in the hot molecular core G31.41+0.31

M. T. Beltrán, R. Cesaroni, V. M. Rivilla +20

As part of our effort to search for circumstellar disks around high-mass stellar objects, we observed the well-known core G31.41+0.31 with ALMA at 1.4 mm with an angular resolution…

astro-ph.SR2018★ 42 cited

On the RR Lyrae stars in globulars: V. the complete Near-Infrared (JHKs) census of omega Centauri RR Lyrae variables

V. F. Braga, P. B. Stetson, G. Bono +35

We present a new complete Near-Infrared (NIR, ) census of RR Lyrae stars (RRLs) in the globular Cen (NGC 5139). We collected 15,472 images with 4-8m class telesc…

astro-ph.SR2018★ 54 cited

Accurate effective temperatures of the metal-poor benchmark stars HD 140283, HD 122563 and HD 103095 from CHARA interferometry

I. Karovicova, T. R. White, T. Nordlander +14

Large stellar surveys of the Milky Way require validation with reference to a set of "benchmark" stars whose fundamental properties are well-determined. For metal-poor benchmark st…