中文
相关论文

相关论文: Recent progress with observations and models to ch…

200 篇论文

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

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

We present our current understanding of the formation and early evolution of protostars, protoplanetary disks, and the driving of outflows as dictated by the interplay of magnetic fields and partially ionized gas in molecular cloud cores.…

太阳与恒星天体物理 · 物理学 2022-09-29 Yusuke Tsukamoto , Anaëlle Maury , Benoît Commerçon , Felipe O. Alves , Erin G. Cox , Nami Sakai , Tom Ray , Bo Zhao , Masahiro N. Machida

Whereas the understanding of most phases of stellar evolution made considerable progress throughout the whole of the twentieth century, stellar formation remained rather enigmatic and poorly constrained by observations until about three…

天体物理学 · 物理学 2015-05-13 J. F. Donati , M. M. Jardine , S. G. Gregory , J. Bouvier , C. Dougados , F. Menard

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

Star formation is a complex process involving the interplay of many physical effects, including gravity, turbulent gas dynamics, magnetic fields and radiation. Our understanding of the process has improved substantially in recent years,…

星系天体物理 · 物理学 2015-05-18 Daniel J. Price , Matthew R. Bate

The role of outflows in the formation of stars and the protostellar disks that generate them is a central question in astrophysics. Outflows are associated with star formation across the entire stellar mass spectrum. In this review, we…

太阳与恒星天体物理 · 物理学 2019-12-13 Ralph E. Pudritz , Tom P. Ray

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

The magnetic field is a key ingredient in the recipe of star formation. Over the past two decades, millimeter and submillimeter interferometers have made major strides in unveiling the role of the magnetic field in star formation at…

太阳与恒星天体物理 · 物理学 2019-03-11 Charles L. H. Hull , Qizhou Zhang

Although protostars and disks are often studied separately owing to numerical and observational challenges, breakthroughs in recent years have highlighted the need to study both objects in concert. The role of magnetic fields in this regard…

太阳与恒星天体物理 · 物理学 2025-04-30 Adnan Ali Ahmad , Matthias González , Patrick Hennebelle , Ugo Lebreuilly , Benoît Commerçon

Truncated abstract: The formation of a protostellar disc is a natural outcome during the star formation process. As gas in a molecular cloud core collapses under self-gravity, the angular momentum of the gas will slow its collapse on small…

太阳与恒星天体物理 · 物理学 2018-12-18 James Wurster , Zhi-Yun Li

The role of magnetic fields in the early stages of star formation is not well constrained. In order to discriminate between different star formation models, we analyze 3D magnetohydrodynamic simulations of low-mass cores and explore the…

星系天体物理 · 物理学 2017-01-18 Joyce W. Y. Lee , Charles L. H. Hull , Stella S. R. Offner

We review theoretical models of the early stages of star formation, in which gravitational collapse is strongly regulated by magnetic fields and the associated process of ambipolar diffusion. We discuss results of numerical simulations and…

天体物理学 · 物理学 2007-05-23 Glenn E. Ciolek , Shantanu Basu

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

(Abridged) Context. Most massive stars are located in multiple stellar systems. Magnetic fields are believed to be essential in the accretion and ejection processes around single massive protostars. Aims. Our aim is to unveil the influence…

太阳与恒星天体物理 · 物理学 2023-05-24 R. Mignon-Risse , M. González , B. Commerçon

Star formation is thought to be triggered by the gravitational collapse of the dense cores of molecular clouds. Angular momentum conservation during the collapse results in the progressive increase of the centrifugal force, which eventually…

地球与行星天体物理 · 物理学 2009-03-11 Raquel Salmeron

Recent theoretical studies have suggested that a magnetic field may play a crucial role in the first star formation in the universe. However, the influence of the magnetic field on the first star formation has yet to be understood well. In…

星系天体物理 · 物理学 2021-05-26 Kenji Eric Sadanari , Kazuyuki Omukai , Kazuyuki Sugimura , Tomoaki Matsumoto , Kengo Tomida

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

Are magnetic fields important in primordial star formation? Assuming that star formation occurs via an accretion disk that is turbulent, initially because of local gravitational instability, we calculate the disk structure for realistic…

天体物理学 · 物理学 2009-11-10 Jonathan C. Tan , Eric G. Blackman

We present first results of our simulations of magnetic fields in the formation of single and binary stars using a recently developed method for incorporating Magnetohydrodynamics (MHD) into the Smoothed Particle Hydrodynamics (SPH) method.…

天体物理学 · 物理学 2009-06-23 Daniel J. Price , Matthew R. Bate
‹ 上一页 1 2 3 10 下一页 ›