output
19922026
Showing 2017 · astro-ph.SRShow all

66 papers · 2 filters

astro-ph.SR2017★ 78 cited

HADES RV Programme with HARPS-N at TNG. VII. Rotation and activity of M-Dwarfs from time-series high-resolution spectroscopy of chromospheric indicators

A. Suárez Mascareño, R. Rebolo, J. I. González Hernández +28

We aim to investigate the presence of signatures of magnetic cycles and rotation on a sample of 71 early M-dwarfs from the HADES RV programme using high-resolution time-series spec…

astro-ph.SR2017★ 32 cited

A view of the H-band light-element chemical patterns in Globular Clusters under the AGB self-enrichment scenario

F. Dell'Agli, D. A. García-Hernández, P. Ventura +7

We discuss the self-enrichment scenario by AGB stars for the formation of multiple populations in globular clusters (GCs) by analyzing data set of giant stars observed in 9 Galacti…

astro-ph.SR2017★ 8 cited

AGB subpopulations in the nearby globular cluster NGC 6397

B. T. MacLean, S. W. Campbell, G. M. De Silva +5

It has been well established that Galactic Globular clusters (GCs) harbour more than one stellar population, distinguishable by the anti-correlations of light element abundances (C…

astro-ph.SR2017★ 12 cited

Infrared spectroscopy of the remnant of Nova Sco 2014: a symbiotic star with too little circumstellar matter to decelerate the ejecta

U. Munari, D. P. K. Banerjee

Pre-outburst 2MASS and WISE photometry of Nova Sco 2014 (V1534 Sco) have suggested the presence of a cool giant at the location of the nova in the sky. The spectral evolution recor…

astro-ph.SR2017★ 50 cited

SN 2017dio: a type-Ic supernova exploding in a hydrogen-rich circumstellar medium

Hanindyo Kuncarayakti, Keiichi Maeda, Christopher J. Ashall +42

SN 2017dio shows both spectral characteristics of a type-Ic supernova (SN) and signs of a hydrogen-rich circumstellar medium (CSM). Prominent, narrow emission lines of H and He are…

astro-ph.SR2017★ 18 cited

The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data

R. Silvotti, S. Schuh, S. -L. Kim +10

V391 Peg (alias HS2201+2610) is a subdwarf B (sdB) pulsating star that shows both p- and g-modes. By studying the arrival times of the p-mode maxima and minima through the O-C meth…