E-LIB Suche - Ergebnisse für: Saffe, C.

1

Disentangling the origin of chemical differences using GHOS:

Saffe, C. ; Miquelarena, P. ; Alacoria, J....
Astronomy & Astrophysics. 682 (2024) - p. L23 , 2024

2

Elemental abundance differences in the massive planet-hosti..:

Flores, M ; Yana Galarza, J ; Miquelarena, P...
Monthly Notices of the Royal Astronomical Society. 527 (2023) 4 - p. 10016-10024 , 2023

Link: https://doi.org/10.1093/..

3

Are Am stars and hot-Jupiter planets related?:

Saffe, C. ; Alacoria, J. ; Miquelarena, P....
Astronomy & Astrophysics. 668 (2022) - p. A157 , 2022

Link: https://doi.org/10.1051/..

4

Discovery of new mercury–manganese stars, including a fast ..:

González, J F ; Nuñez, N E ; Saffe, C...
Monthly Notices of the Royal Astronomical Society. 502 (2021) 3 - p. 3670-3684 , 2021

Link: https://doi.org/10.1093/..

5

ζ1 + ζ2 Reticuli binary system: a puzzling chromospheric ac..:

Flores, M ; Saffe, C ; Buccino, A...
Monthly Notices of the Royal Astronomical Society. 476 (2018) 2 - p. 2751-2759 , 2018

Link: https://doi.org/10.1093/..

6

The magnetic field in HD 161701, the only binary system ide..:

Hubrig, S. ; Carroll, T. A. ; González, J. F....
Monthly Notices of the Royal Astronomical Society: Letters. 440 (2014) 1 - p. L6-L10 , 2014

Link: https://doi.org/10.1093/..

7

Elemental abundances differences in the massive planet-host..:

Flores, M ; Galarza, J. Yana ; Miquelarena, P...
http://arxiv.org/abs/2311.17272. , 2023

Link: http://arxiv.org/abs/231..

8

Are Am stars and hot-Jupiter planets related?:

Saffe, C ; Alacoria, J ; Miquelarena, P...
http://arxiv.org/abs/2209.14257. , 2022

Link: http://arxiv.org/abs/220..

9

Testing the accretion scenario of lambda Boo stars:

Alacoria, J ; Saffe, C ; Arancibia, M. Jaque...
http://arxiv.org/abs/2202.05066. , 2022

Link: http://arxiv.org/abs/220..

10

Chemical analysis of early-type stars with planets:

Saffe, C ; Miquelarena, P ; Alacoria, J...
http://arxiv.org/abs/2101.04416. , 2021

Link: http://arxiv.org/abs/210..

11

Detecting prolonged activity minima in binary stars. The ca..:

Flores, M ; Arancibia, M. Jaque ; Bustos, R. V. Ibañez...
http://arxiv.org/abs/2012.08983. , 2020

Link: http://arxiv.org/abs/201..

12

KELT-17: a chemically peculiar Am star and a hot-Jupiter pl..:

Saffe, C ; Miquelarena, P ; Alacoria, J...
http://arxiv.org/abs/2007.14210. , 2020

Link: http://arxiv.org/abs/200..

13

High-precision analysis of binary stars with planets. I. Se..:

Saffe, C ; Jofre, E ; Miquelarena, P...
http://arxiv.org/abs/1904.01955. , 2019

Link: http://arxiv.org/abs/190..

14

Gemini-GRACES high-quality spectra of Kepler evolved stars ..:

Jofré, E ; Almenara, J. M ; Petrucci, R...
http://arxiv.org/abs/1912.10278. , 2019

Link: http://arxiv.org/abs/191..

15

Using non-solar-scaled opacities to derive stellar paramete..:

Saffe, C ; Flores, M ; Miquelarena, P...
http://arxiv.org/abs/1809.09250. , 2018

Link: http://arxiv.org/abs/180..