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Deriving Iodine-free Spectra for High-resolution Echelle Spectrographs
(Institute of Physics Publishing, 2019)
We describe a new method to derive clean, iodine-free spectra directly from observations acquired using high-resolution echelle spectrographs equipped with iodine cells. The main motivation to obtain iodine-free spectra ...
High resolution study of 104Pd(d,t)103Pd
(Sociedade Brasileira de Física, 2008)
Information collected in the present high resolution study of 104Pd(d,t)103Pd is interpreted within the systematics of the A ~ 100 region. The paper complements data previously presented by the S.Paulo Group, which were ...
High-resolution measurements of low-energy conversion electrons
(Springer, 2000-08)
High-resolution measurements of low-energy conversion electrons have been performed in odd and odd-odd nuclei with masses around A = 182. The experimental setup, a magnetic spectrograph coupled to a specific tape transport ...
Remedición de valores Q0 de reacciones nucleares entre los elementos ligeros
(Revista Mexicana de Física, 2009)
Magnetic field detection in the bright A0-type supergiant HD 92207
(EDP Sciences, 2012-10)
Context. Recent developments in observational techniques and theories revealed the potential significance of magnetic fields for stellar structure, evolution, and circumstellar environment. At present, the distribution of ...
Magnetic variability in the young solar analog KIC 10644253: observations from the Kepler satellite and the HERMES spectrograph
(EDP Sciences, 2016-02-29)
The continuous photometric observations collected by the Kepler satellite over 4 yr provide a wealth of data with an unequalled quantity and quality for the study of stellar evolution of more than 200 000 stars. Moreover, ...
Analisis químico empleando protones con energías de1.5 Mev
(Revista Mexicana de Física, 2009)
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars
(EDP Sciences, 2013-03)
Context. Theories on the origin of magnetic fields in massive stars
remain poorly developed, because the properties of their magnetic field
as function of stellar parameters could not yet be investigated.
Additional ...
New spectroscopic and polarimetric observations of the A0 supergiant HD 92207
(Wiley, 2015-02)
Our recent search for the presence of a magnetic field in the bright earlyA-type supergiant HD92207 using FORS2 in spectropolarimetric mode revealed thepresence of a longitudinal magnetic field of the order of a few hundred ...
The HERMES solar atlas and the spectroscopic analysis of the seismic solar analogue KIC 3241581
(EDP Sciences, 2015-11-18)
Context. Solar-analogue stars provide an excellent resource to study the Sun’s evolution, i.e. the changes with time in stellar structure, activity, or rotation for solar-like stars. The unparalleled photometric data from ...