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Though widely observed to be emanating out from a variety of galactic and extra-galactic sources, the underlying physical mechanism behind the formation of the cosmic jets and outflows are wrapped around by the veil of mystery till date.…

天体物理学 · 物理学 2007-05-23 Tapas K. Das

Active galaxies and quasers are believed to harbour Black Holes at their centers and at the same time produce cosmic radio jets through which immense amount of matter and energy are ejected out of the core of the galaxy. In our work we…

天体物理学 · 物理学 2007-05-23 Tapas K. Das

Observational advances over the last decade reveal that star formation is associated with the simultaneous presence of gravitationally collapsing gas, bipolar outflow, and an accretion disk. Two theoretical views of star formation suppose…

天体物理学 · 物理学 2007-05-23 R. E. Pudritz , D. E. McLaughlin , R. Ouyed

Outflows are common in many astrophysical systems which contain black holes and neutron stars. Difference between stellar outflows and outflows from these systems is that the outflows in these systems have to form out of the inflowing…

天体物理学 · 物理学 2007-05-23 Sandip K. Chakrabarti

I review accretion and outflow in active galactic nuclei. Accretion appears to occur in a series of very small--scale, chaotic events, whose gas flows have no correlation with the large--scale structure of the galaxy or with each other. The…

宇宙学与河外天体物理 · 物理学 2015-05-18 Andrew King

Outflows are common in many astrophysical systems which contain black holes and neutron stars. Difference between stellar outflows and outflows from these systems is that the outflows in these systems have to form out of the inflowing…

天体物理学 · 物理学 2007-05-23 Sandip K. Chakrabarti

We compute mass outflow rates from accretion disks around compact objects, such as neutron stars and black holes. These computations are done using combinations of exact transonic inflow and outflow solutions which may or may not form…

天体物理学 · 物理学 2009-10-31 Tapas K. Das , Sandip K. Chakrabarti

Recent observations have revealed massive galactic molecular outflows that may have physical conditions (high gas densities) required to form stars. Indeed, several recent models predict that such massive galactic outflows may ignite star…

The relation between the mass accretion rate onto the circumstellar disc and the rate of mass ejection by magnetically driven winds is investigated using three-dimensional magnetohydrodynamics simulations. Using a spherical cloud core with…

太阳与恒星天体物理 · 物理学 2017-07-05 Yuko Matsushita , Masahiro N. Machida , Yuya Sakurai , Takashi Hosokawa

Interstellar ultraviolet absorption-lines provide crucial information about the properties of galactic outflows. In this paper, we augment our previous analysis of the systematic properties of starburst-driven galactic outflows by expanding…

星系天体物理 · 物理学 2016-05-04 Timothy M. Heckman , Sanchayeeta Borthakur

Galactic outflows are believed to play an important role in regulating star formation in galaxies, but estimates of the outflowing mass and momentum have historically been based on uncertain assumptions. Here, we measure the mass, momentum,…

星系天体物理 · 物理学 2017-06-28 John Chisholm , Christy A. Tremonti , Claus Leitherer , Yanmei Chen

Research in recent decades has seen many important advances in understanding the role of jets and outflows in the star formation process. Although, many open issues still remain, multi-wavelength high resolution observations have provided…

星系天体物理 · 物理学 2011-12-13 Deirdre Coffey

We examine the effects of galaxy outflows on the formation of dwarf galaxies in numerical simulations of the high-redshift Universe. Using a Smoothed Particle Hydrodynamic code, we conduct two detailed simulations of a (5.2 Mpc/h)^3…

天体物理学 · 物理学 2009-10-31 Evan Scannapieco , Robert J. Thacker , Marc Davis

Numerical simulations have become a major tool for understanding galaxy formation and evolution. Over the decades the field has made significant progress. It is now possible to simulate the formation of individual galaxies and galaxy…

星系天体物理 · 物理学 2017-08-30 Thorsten Naab , Jeremiah P. Ostriker

Outflows and jets are intimately related to the formation of stars, and play an important role in redistributing mass, energy and angular momentum within the dense core and parent cloud. The interplay between magnetic field and rotation is…

太阳与恒星天体物理 · 物理学 2015-05-19 Andrea Ciardi , Patrick Hennebelle

Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far. They operate over the full extent of their galaxy hosts, from the innermost regions of galactic nuclei to the outermost reaches of galaxy halos. They…

星系天体物理 · 物理学 2020-04-15 Sylvain Veilleux , Roberto Maiolino , Alberto D. Bolatto , Susanne Aalto

We investigate how magnetically driven outflows are powered by a rotating, weakly magnetized accretion flow onto a supermassive black hole using axisymmetric magnetohydrodynamic simulations. Our proposed model focuses on the accretion…

星系天体物理 · 物理学 2022-02-16 Shinsuke Takasao , Yuri Shuto , Keiichi Wada

During their birth all stars undergo periods of copious mass loss, frequently characterized by the occurrence of bipolar outflows. These outflows are believed to play a fundamental role in the star formation process. However the exact…

天体物理学 · 物理学 2007-05-23 Derek E. Bretherton , Toby J. T. Moore , Naomi A. Ridge

Different mechanisms can drive outflows in active galactic nuclei (AGN), but it is often unclear which mechanism dominates, if any. To quantify the impact of AGN feedback on galaxy evolution, the driving mechanism of outflows must be better…

星系天体物理 · 物理学 2018-03-01 Dominika Wylezalek , Raffaella Morganti

We compute mass outflow rates from advective accretion disks around compact objects, such as neutron stars and black holes. These computations, for the first time, are done using combinations of exact transonic inflow and outflow solutions…

天体物理学 · 物理学 2007-05-23 Tapas K. Das , Sandip K. Chakrabarti
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