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相关论文: The Role of Magnetic Fields in Setting the Star Fo…

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Star formation in the centers of galaxies is thought to yield massive stars with a possibly top-heavy stellar mass distribution. It is likely that magnetic fields play a crucial role in the distribution of stellar masses inside star-forming…

星系天体物理 · 物理学 2012-08-03 S. Hocuk , D. R. G. Schleicher , M. Spaans , S. Cazaux

Magnetic fields play an important role for the formation of stars in both local and high-redshift galaxies. Recent studies of dynamo amplification in the first dark matter haloes suggest that significant magnetic fields were likely present…

星系天体物理 · 物理学 2020-07-08 Piyush Sharda , Christoph Federrath , Mark R. Krumholz

In this chapter we review recent advances in understanding the roles that magnetic fields play throughout the star formation process, gained through observations and simulations of molecular clouds, the dense, star-forming phase of the…

星系天体物理 · 物理学 2022-03-22 Kate Pattle , Laura Fissel , Mehrnoosh Tahani , Tie Liu , Evangelia Ntormousi

The regulation of galactic-scale star formation rates (SFRs) is a basic problem for theories of galaxy formation and evolution: which processes are responsible for making observed star formation rates so inefficient compared to maximal…

星系天体物理 · 物理学 2015-06-23 Sven Van Loo , Jonathan C. Tan , Sam A. E. G. Falle

We review the role that magnetic field may have on the formation and evolution of molecular clouds. After a brief presentation and main assumptions leading to ideal MHD equations, their most important correction, namely the ion-neutral…

星系天体物理 · 物理学 2019-02-05 Patrick Hennebelle , Shu-ichiro Inutsuka

We examine the effect of magnetic fields on star cluster formation by performing simulations following the self-gravitating collapse of a turbulent molecular cloud to form stars in ideal MHD. The collapse of the cloud is computed for global…

天体物理学 · 物理学 2009-11-13 Daniel Price , Matthew Bate

Magnetic fields are important at every scale in the star formation process: from the dynamics of the ISM in galaxies, to the collapse of turbulent molecular clouds to form stars and in the fragmentation of individual star forming cores. The…

天体物理学 · 物理学 2008-04-30 Daniel J. Price , Matthew R. Bate , Clare L. Dobbs

We investigate the effects of magnetic fields and radiative protostellar feedback on the star formation process using self-gravitating radiation magnetohydrodynamical calculations. We present results from a series of calculations of the…

太阳与恒星天体物理 · 物理学 2015-05-13 Daniel J. Price , Matthew R. Bate

Massive stars disproportionately influence their surroundings. How they form has only started to become clear recently through radiation gas dynamical simulations. However, until now, no simulation has simultaneously included both magnetic…

太阳与恒星天体物理 · 物理学 2015-03-17 Thomas Peters , Robi Banerjee , Ralf S. Klessen , Mordecai-Mark Mac Low

The measured star-formation rates (SFRs) of galaxies comprise an important constraint on galaxy evolution and also on their cosmological boundary conditions. Any available tracer of the SFR depends on the shape of the mass-distribution of…

星系天体物理 · 物理学 2021-12-22 Pavel Kroupa , Tereza Jerabkova

The question whether magnetic fields play an important role in the processes of molecular cloud and star formation has been debated for decades. Recent observations have revealed a simple picture that may help illuminate these questions:…

星系天体物理 · 物理学 2015-06-19 Hua-bai Li , Alyssa Goodman , T. K. Sridharan , Martin Houde , Zhi-Yun Li , Giles Novak , Kwok Sun Tang

Magnetic fields are often invoked as playing a primary role in star formation and in the formation of high-mass stars. We investigate the effect of magnetic fields on the formation of high-mass cores using the 3-dimensional smoothed…

星系天体物理 · 物理学 2025-04-04 Katerina Sophia Klos , Ian A. Bonnell , Rowan J. Smith

While magnetic fields are important in contemporary star formation, their role in primordial star formation is unknown. Magnetic fields of order 10^-16 G are produced by the Biermann battery due to the curved shocks and turbulence…

星系天体物理 · 物理学 2020-07-15 Christopher F. McKee , Athena Stacy , Pak Shing Li

Understanding star formation rates (SFR) is a central goal of modern star-formation models, which mainly involve gravity, turbulence and, in some cases, magnetic fields (B-fields). However, a connection between B-fields and SFR has never…

星系天体物理 · 物理学 2017-06-27 Hua-bai Li , Hangjin Jiang , Xiaodan Fan , Qilao Gu , Yapeng Zhang

One of the key mysteries of star formation is the origin of the stellar initial mass function (IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and significant variations are only inferred in extreme…

During the past decade the dynamical importance of magnetic fields in molecular clouds has been increasingly recognized, as observational evidence has accumulated. However, how a magnetic field affect star formation is still unclear.…

星系天体物理 · 物理学 2020-09-15 C. Y. Law , H. -b. Li , Z. Cao , C. -Y. Ng

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

We review star formation in molecular clouds and describe why magnetic fields may be important and how they can influence filamentary structure and the column density probability distribution function (PDF). We also comment on the origin of…

星系天体物理 · 物理学 2017-10-18 Shantanu Basu , Sayantan Auddy

Magnetic fields play an important role in the dynamics of present-day molecular clouds. Recent work has shown that magnetic fields are equally important for primordial clouds, which form the first stars in the Universe. While the primordial…

星系天体物理 · 物理学 2021-02-24 Piyush Sharda , Christoph Federrath , Mark R. Krumholz , Dominik R. G. Schleicher

Recent cosmological hydrodynamic simulations have suggested that the first stars in the universe often form as binary or multiple systems. However, previous studies typically overlooked the potential influence of magnetic fields during this…

星系天体物理 · 物理学 2024-05-27 Kenji Eric Sadanari , Kazuyuki Omukai , Kazuyuki Sugimura , Tomoaki Matsumoto , Kengo Tomida
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