output
20092026
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations

Showing 2018 · astro-ph.SRShow all

9 papers · 2 filters

astro-ph.SR2018★ 7 cited

Quest for the Donor Star in the Magnetic Precataclysmic Variable V1082 Sgr

G. Tovmassian, J. F. Gonzalez, M. -S. Hernandez +3

We obtained high-resolution spectra and multicolor photometry of V1082 Sgr to study the donor star in this 20.8 hr orbital period binary, which is assumed to be a detached system.…

astro-ph.SR2018★ 10 cited

Physical processes involved in the EUV "Surge" Event of 09 May 2012

Marcelo López Fuentes, Cristina H. Mandrini, Mariano Poisson +4

We study an EUV confined ejection observed on 09 May 2012 in active region (AR) NOAA 11476. For the analysis we use observations in multiple wavelengths (EUV, X-rays, H, and mag…

astro-ph.SR2018★ 14 cited

Using non-solar-scaled opacities to derive stellar parameters. Toward high-precision parameters and abundances

C. Saffe, M. Flores, P. Miquelarena +5

We implemented non-solar-scaled opacities in a simultaneous derivation of fundamental parameters and abundances. We carried out a high-precision stellar parameters and abundance de…

astro-ph.SR2018★ 17 cited

HD 38858: a solar type star with a 10.8 yr activity cycle. Searching for Balmer and metallic line variations

M. Flores, J. F. González, M. Jaque Arancibia +5

Context. The detection of chromospheric activity cycles in solar-analogue and twin stars, can be used to put in context the solar cycle. However, there is a relatively low percenta…

astro-ph.SR2018★ 6 cited

HD 149277: a rare short-period SB2 system with a subsynchronously rotating magnetic He-rich primary

J. F. González, S. Hubrig, S. P. Järvinen +1

HD 149277 is a rare SB2 system with a slowly rotating magnetic He-rich primary with d. The CFHT/ESPaDOnS archive spectra revealed $P_{\rm orb}=11.5192 \pm 0.0005…

astro-ph.SR2018★ 134 cited

On the evolution of ultra-massive white dwarfs

María E. Camisassa, Leandro G. Althaus, Alejandro H. Córsico +6

Ultra-massive white dwarfs are powerful tools to study various physical processes in the Asymptotic Giant Branch (AGB), type Ia supernova explosions and the theory of crystallizati…

astro-ph.SR2018★ 12 cited

On the nature of the black-body stars

Aldo Serenelli, Rene Rohrmann, Masataka Fukugita

A selection of 17 stars in the Sloan Digital Sky Survey, previously identified as DC class white dwarfs (WDs), has been reported to show spectra very close to blackbody radiation i…

astro-ph.SR2018★ 5 cited

Reticuli binary system: A puzzling chromospheric activity pattern

M. Flores, C. Saffe, A. Buccino +4

We perform, for the first time, a detailed long-term activity study of the binary system Ret. We use all available HARPS spectra obtained between the years 2003 and 2016. We bu…

astro-ph.SR2018★ 21 cited

X-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Cru

G. J. M. Luna, K. Mukai, J. L. Sokoloski +8

Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries in which red giants transfer material to white dwarfs (WDs) has been difficult to…