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相关论文: Magnetic fields in massive spirals: The role of fe…

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What exactly controls star formation in the Galaxy remains controversial. In particular, the role of feedback and magnetic field are still partially understood. We investigate the role played by supernovae feedback and magnetic field onto…

星系天体物理 · 物理学 2015-06-19 Patrick Hennebelle , Olivier Iffrig

Magnetic fields constitute an energetic component of the interstellar medium in galaxies and hence can affect the formation of galactic structures. Sensitive resolved radio continuum observations together with statistical studies in galaxy…

星系天体物理 · 物理学 2018-11-20 Fatemeh S. Tabatabaei

The origin and evolution of magnetic fields in the Universe is still an open question. Their observations in galaxies suggest strong magnetic fields already at high redshift as well as at present time. However, neither primordial magnetic…

星系天体物理 · 物理学 2017-04-21 Michael Rieder , Romain Teyssier

At metallicities lower than that of the Small Magellanic Cloud, it remains essentially unexplored how fossil magnetic fields, forming large-scale magnetospheres, could affect the evolution of massive stars, thereby impacting the fundamental…

太阳与恒星天体物理 · 物理学 2024-07-31 Z. Keszthelyi , J. Puls , G. Chiaki , H. Nagakura , A. ud-Doula , T. Takiwaki , N. Tominaga

As one of the prime contributors to the interstellar medium energy budget, magnetic fields naturally play a part in shaping the evolution of galaxies. Galactic magnetic fields can originate from strong primordial magnetic fields provided…

星系天体物理 · 物理学 2020-06-03 Sergio Martin-Alvarez , Adrianne Slyz , Julien Devriendt , Carlos Gómez-Guijarro

Magnetic fields play a vital role in numerous astrophysical processes such as star formation and the interstellar medium. In particular, their role in the formation and evolution of galaxies is not well understood. This paper presents…

星系天体物理 · 物理学 2021-12-10 Huai-Hsuan Chiu , Ke-Jung Chen

Magnetic fields in nearby, star-forming galaxies reveal both large-scale patterns and small-scale structures. A large-scale field reversal may exist in the Milky Way but no such reversals have been observed so far in external galaxies. The…

星系天体物理 · 物理学 2015-05-30 David Moss , Rodion Stepanov , Tigran Arshakian , Rainer Beck , Marita Krause , Dmitri Sokoloff

We study the cosmic evolution of the magnetic fields of a large sample of spiral galaxies in a cosmologically representative volume by employing a semi-analytic galaxy formation model and numerical dynamo solver in tandem. We start by…

星系天体物理 · 物理学 2019-01-03 Luiz Felippe S. Rodrigues , Luke Chamandy , Anvar Shukurov , Carlton M. Baugh , A. Russ Taylor

Massive stars are crucial building blocks of galaxies and the universe, as production sites of heavy elements and as stirring agents and energy providers through stellar winds and supernovae. The field of magnetic massive stars has seen…

太阳与恒星天体物理 · 物理学 2015-05-27 Rolf Walder , Doris Folini , Georges Meynet

Magnetic fields permeate the Universe on all scales and play a key role during star formation. We study the evolution of magnetic fields around a massive metal-free (Population III) star at $z \sim 15$ during the growth of its HII region…

星系天体物理 · 物理学 2016-08-03 Daegene Koh , John H. Wise

Magnetic fields play a crucial role at all stages of the formation of low mass stars and planetary systems. In the final stages, in particular, they control the kinematics of in-falling gas from circumstellar discs, and the launching and…

太阳与恒星天体物理 · 物理学 2015-05-19 S. G. Gregory , M. Jardine , C. G. Gray , J. -F. Donati

Magnetic field is playing an important role at all stages of star evolution from star formation to the endpoints. The main effects are briefly reviewed. We also show that O-type stars have large convective envelopes, where convective dynamo…

天体物理学 · 物理学 2009-11-13 André Maeder , Georges Meynet , Cyril Georgy , Sylvia Ekström

Large-scale dipolar surface magnetic fields have been detected in a fraction of OB stars, however only few stellar evolution models of massive stars have considered the impact of these fossil fields. We are performing 1D hydrodynamical…

太阳与恒星天体物理 · 物理学 2017-11-15 Z. Keszthelyi , G. A. Wade , V. Petit

The universe is magnetized on all scales probed so far. On the largest scales, galaxies and galaxy clusters host magnetic fields at the micro Gauss level coherent on scales up to ten kpc. Recent observational evidence suggests that even the…

宇宙学与河外天体物理 · 物理学 2017-05-26 Kandaswamy Subramanian

Surface magnetic fields have a strong impact on stellar mass loss and rotation and, as a consequence, on the evolution of massive stars. In this work we study the influence of an evolving dipolar surface fossil magnetic field with an…

太阳与恒星天体物理 · 物理学 2019-03-27 Z. Keszthelyi , G. Meynet , C. Georgy , G. A. Wade , V. Petit , A. David-Uraz

We numerically simulate some of the most critical physical processes in galaxy formation: The supernova feedback, in conjunction with gasdynamics and gravity, plays a crucial role in determining how galaxies arise within the context of a…

天体物理学 · 物理学 2015-06-24 G. Yepes , R. Kates , A. Khokhlov , A. Klypin

Over the last decade, tremendous strides have been achieved in our understanding of magnetism in main sequence hot stars. In particular, the statistical occurrence of their surface magnetism has been established (~10%) and the field origin…

Magnetic fields on a range of scales play a large role in the ecosystems of galaxies, both in the galactic disk and in the extended layers of gas away from the plane. Observing magnetic field strength, structure and orientation is complex,…

星系天体物理 · 物理学 2015-05-27 Marijke Haverkorn , Volker Heesen

We use cosmological simulations in order to study the effects of supernova (SN) feedback on the formation of a Milky Way-type galaxy of virial mass ~10^12 M_sun/h. We analyse a set of simulations run with the code described by Scannapieco…

天体物理学 · 物理学 2009-11-13 Cecilia Scannapieco , Patricia B. Tissera , Simon D. M. White , Volker Springel

Magnetic fields are believed to play an important role in the evolution of molecular clouds, from their large scale structure to dense cores, protostellar envelopes, and protoplanetary disks. How important is unclear, and whether magnetic…

天体物理学 · 物理学 2007-05-23 Tyler L. Bourke , Alyssa A. Goodman
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