Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Dieter H. Nickeler"'
Autor:
Dieter H. Nickeler, Michaela Kraus
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 131 (2024)
Structures in circumstellar matter reflect both fast processes and quasi-equilibrium states. A geometrical diversity of emitting circumstellar matter is observed around evolved massive stars, in particular around B[e] supergiants. We recapitulate cla
Externí odkaz:
https://doaj.org/article/973fe8cab0c9470182af20d95f5d6cad
Publikováno v:
Galaxies, Vol 11, Iss 3, p 76 (2023)
Massive stars expel large amounts of mass during their late evolutionary phases. We aim to unveil the physical conditions within the warm molecular environments of B[e] supergiants (B[e]SGs) and yellow hypergiants (YHGs), which are known to be embedd
Externí odkaz:
https://doaj.org/article/dec091d0e4e74470b0a4093f95551293
Autor:
Alexei Moiseev, David O. Jones, Dieter H. Nickeler, Julieta Paz Sánchez Arias, Lydia Sonia Cidale, T. Liimets, Michaela Kraus
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The Astronomical Journal
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The Astronomical Journal
The Galactic B[e] supergiant MWC 137 is surrounded by a large-scale optical nebula. To shed light on the physical conditions and kinematics of the nebula, we analyze the optical forbidden emission lines [NII] 6548,6583 and [SII] 6716,6731 in long-sli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50ded3c1d8e2a5ebe95f41b0a1079ad0
Topological characteristics reveal important physical properties of plasma structures and astrophysical processes. Physical parameters and constraints are linked with topological invariants, which are important for describing magnetic reconnection sc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7487746a01db155d864ff7c7b115b14c
Many magnetic structures in the solar atmosphere evolve rather slowly so that they can be assumed as (quasi-)static or (quasi-)stationary and represented via magneto-hydrostatic (MHS) or stationary magneto-hydrodynamic (MHD) equilibria, respectively.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73527c6356e3784cb02a64ec32f4a9a1
Autor:
Grigoris Maravelias, Michel Curé, M. Borges Fernandes, R. Vallverdú, Rodolfo H. Barbá, M. L. Arias, Dieter H. Nickeler, Manfred Kraus, Lydia Sonia Cidale, Anna Aret, Andrea Fabiana Torres
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Context. B[e] supergiants are evolved massive stars, enshrouded in a dense wind and surrounded by a molecular and dusty disk. The mechanisms that drive phases of enhanced mass loss and mass ejections, responsible for the shaping of the circumstellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0e321630513ddf9409dcabd60a4624f
Autor:
Dieter H. Nickeler, Marian Karlický
Publikováno v:
Astrophysics and Space Sciences Transactions. 2:63-72
This article discusses and tests the validity of the frozen in magnetic field paradigm (or 'ideal magnetohydro- dynamics (MHD) constraint') which is usually adopted by many authors dealing with heliospheric physics. To show the problem of using ideal
Autor:
Grigoris Maravelias, Dieter H. Nickeler, D. S. Gunawan, Michel Curé, Cristina Elisabet Cappa, N. U. Duronea, T. Liimets, Miguel Santander-García, Mary E. Oksala, M. L. Arias, Lydia Sonia Cidale, Michaela Kraus, Marcelo Borges Fernandes
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2017, 154 (5), pp.186. ⟨10.3847/1538-3881/aa8df6⟩
The Astronomical Journal, 2017, 154 (5), pp.186. ⟨10.3847/1538-3881/aa8df6⟩
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2017, 154 (5), pp.186. ⟨10.3847/1538-3881/aa8df6⟩
The Astronomical Journal, 2017, 154 (5), pp.186. ⟨10.3847/1538-3881/aa8df6⟩
The Galactic object MWC 137 has been suggested to belong to the group of B[e] supergiants. However, with its large-scale optical bipolar ring nebula and high-velocity jet and knots, it is a rather atypical representative of this class. We performed m
Autor:
Dieter H. Nickeler, Michel Curé, Marcelo Borges Fernandes, S. Tomic, Lydia Sonia Cidale, Michaela Kraus, R. O. J. Venero, M. Haucke
During the post-main sequence evolution massive stars pass through several short-lived phases, in which they experience enhanced mass loss in the form of clumped winds and mass ejection events of unclear origin. The discovery that stars populating th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e24c7110c1a6b1baabca3529d81a4c23
http://arxiv.org/abs/1309.4904
http://arxiv.org/abs/1309.4904
Publikováno v:
Astronomy & Astrophysics. 556:A61
We consider a magnetic configuration consisting of an arcade structure and a detached plasmoid, resulting from a magnetic reconnection process, as is typically found in connection with solar flares. We study spontaneous current fragmentation caused b