The Kepler characterization of the variability among A-and F-type stars-I. General overview

K Uytterhoeven, A Moya, A Grigahcène… - Astronomy & …, 2011 - aanda.org
Context. The Kepler spacecraft is providing time series of photometric data with
micromagnitude precision for hundreds of AF type stars. Aims. We present a first general …

Solar system abundances and condensation temperatures of the halogens fluorine, chlorine, bromine, and iodine

K Lodders, B Fegley Jr - Geochemistry, 2023 - Elsevier
We review a large body of available meteoritic and stellar halogen data in the literature used
for solar system abundances (ie, representative abundances of the solar system at the time …

A high-resolution spectropolarimetric survey of Herbig Ae/Be stars–I. Observations and measurements

E Alecian, GA Wade, C Catala… - Monthly Notices of …, 2013 - academic.oup.com
This is the first in a series of papers in which we describe and report the analysis of a large
survey of Herbig Ae/Be stars in circular spectropolarimetry. Using the ESPaDOnS and …

Spiral arms in disks: planets or gravitational instability?

R Dong, JR Najita, S Brittain - The Astrophysical Journal, 2018 - iopscience.iop.org
Spiral arm structures seen in scattered-light observations of protoplanetary disks can
potentially serve as signposts of planetary companions. They can also lend unique insights …

The GAPS Programme with HARPS-N at TNG-XIX. Atmospheric Rossiter-McLaughlin effect and improved parameters of KELT-9b

F Borsa, M Rainer, AS Bonomo, D Barbato… - Astronomy & …, 2019 - aanda.org
Aims. In the framework of the GAPS project, we observed the planet-hosting star KELT-9 (A-
type star, v sin i~ 110 km s− 1) with the HARPS-N spectrograph at the Telescopio Nazionale …

Chemical abundances of magnetic and non-magnetic Herbig Ae/Be stars

CP Folsom, S Bagnulo, GA Wade… - Monthly Notices of …, 2012 - academic.oup.com
The photospheres of about 10–20 per cent of main-sequence A-and B-type stars exhibit a
wide range of chemical peculiarities, often associated with the presence of a magnetic field …

NLTE Line Formation for Mg i and Mg ii in the Atmospheres of B–A–F–G–K Stars

S Alexeeva, T Ryabchikova… - The Astrophysical …, 2018 - iopscience.iop.org
Non-local thermodynamical equilibrium (NLTE) line formation for Mg i and Mg ii lines is
considered in classical 1D LTE model atmospheres of the Sun and 17 stars with reliable …

A non-local thermodynamical equilibrium line formation for neutral and singly ionized titanium in model atmospheres of reference A–K stars

TM Sitnova, LI Mashonkina… - Monthly Notices of the …, 2016 - academic.oup.com
We construct a model atom for Ti i–ii using more than 3600 measured and predicted energy
levels of Ti i and 1800 energy levels of Ti ii, and quantum mechanical photoionization cross …

Non-local thermodynamic equilibrium line formation for Si iiiiii in A–B stars and the origin of Si ii emission lines in ι Her

L Mashonkina - Monthly Notices of the Royal Astronomical …, 2020 - academic.oup.com
ABSTRACT A comprehensive model atom was developed for Si i–ii–iii using the most up-to-
date atomic data available so far. Based on non-local thermodynamic equilibrium (NLTE) …

A detailed spectropolarimetric analysis of the planet-hosting star WASP-12

L Fossati, S Bagnulo, A Elmasli… - The Astrophysical …, 2010 - iopscience.iop.org
The knowledge of accurate stellar parameters is paramount in several fields of stellar
astrophysics, particularly in the study of extrasolar planets, where often the star is the only …