An investigation of the rotational properties of magnetic chemically peculiar stars

M Netopil, E Paunzen, S Hümmerich… - Monthly Notices of the …, 2017 - academic.oup.com
The magnetic chemically peculiar (mCP) stars of the upper main sequence exhibit strong,
globally organized magnetic fields that are inclined to the rotational axis and facilitate the …

The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud – Point source classification I

PM Woods, JM Oliveira, F Kemper… - Monthly Notices of …, 2011 - academic.oup.com
We present the classification of 197 point sources observed with the Infrared Spectrograph
in the SAGE-Spec Legacy programme on the Spitzer Space Telescope. We introduce a …

Chemically peculiar stars and their temperature calibration

M Netopil, E Paunzen, HM Maitzen, P North… - Astronomy & …, 2008 - aanda.org
Aims. The determination of effective temperature for chemically peculiar (CP) stars by means
of photometry is a sophisticated task due to their abnormal colours. Standard calibrations for …

Inhibition of thermohaline mixing by a magnetic field in Ap star descendants: implications for the Galactic evolution of 3He

C Charbonnel, JP Zahn - Astronomy & Astrophysics, 2007 - aanda.org
Aims. To reconcile the measurements of 3 He/H in Galactic HII regions with high values of 3
He in a couple of planetary nebulae, we propose that thermohaline mixing is inhibited by a …

The (non-) variability of magnetic chemically peculiar candidates in the Large Magellanic Cloud

E Paunzen, Z Mikulášek, R Poleski, J Krtička… - Astronomy & …, 2013 - aanda.org
Context. The galactic magnetic chemically peculiar (mCP) stars of the upper main sequence
are well known as periodic spectral and light variables. The observed variability is obviously …

New spectroscopic classifications of 35 chemically peculiar candidate stars

E Paunzen, M Netopil, OI Pintado… - Astronomische …, 2011 - Wiley Online Library
The chemically peculiar (CP) stars of the upper main sequence are perfect tracers for
several astrophysical processes. Their study especially in open clusters further helps to …

The first Δa observations of three globular clusters

E Paunzen, IK Iliev, OI Pintado, H Baum… - Monthly Notices of …, 2014 - academic.oup.com
Globular clusters are main astrophysical laboratories to test and modify evolutionary models.
Thought to be rather homogeneous in their local elemental distribution of members, results …

Stars with a stable magnetic field

L Ferrario - arXiv preprint arXiv:1801.09368, 2018 - arxiv.org
In this review, I will summarise what we know about magnetic fields in stars and what the
origin of these magnetic fields may be. I will address the issue of whether the magnetic flux …

A search for peculiar stars in the open cluster Hogg 16

S Cariddi, NM Azatyan, P Kurfürst, L Štofanová… - New Astronomy, 2018 - Elsevier
The study of chemically peculiar (CP) stars in open clusters provides valuable information
about their evolutionary status. Their detection can be performed using the Δa photometric …

[PDF][PDF] What can we expect from a census of Ap stars in open star clusters in the Galaxy and beyond?

HM Maitzen, E Paunzen, M Netopil - Contrib. Astron. Obs. Skalnaté …, 2008 - academia.edu
We discuss the presence of magnetic peculiar stars in open clusters on the basis of
photometric identification, in a sample that covers not only the solar neighbourhood but also …