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Jets are a ubiquitous part of the accretion process, seen in a wide variety of objects ranging from active galaxies (AGN) to X-ray binary stars and even newly formed stars. AGN jets are accelerated by the supermassive black hole of their…

Stars captured by black holes (BHs) can be torn apart by strong tidal forces, producing electromagnetic flares. To date, more than 100 tidal disruption events (TDEs) have been observed, each involving invariably normal gaseous stars whose…

We present time-series VLT spectroscopy and NTT photometry of the cataclysmic variable SDSS J220553.98+115553.7, which contains a pulsating white dwarf. We determine a spectroscopic orbital period of 82.825 +/- 0.089 min from velocity…

天体物理学 · 物理学 2009-11-13 John Southworth , D W Townsley , B T Gaensicke

The recently discovered high-energy transient Swift J164449.3+573451 (Sw J1644+57) is thought to arise from the tidal disruption of a passing star by a dormant massive black hole. Modeling of the broadband emission suggests the presence of…

高能天体物理现象 · 物理学 2015-05-28 Xiang-Yu Wang , Ruo-Yu Liu , Zi-Gao Dai , K. S. Cheng

We compare some of the properties of rapid oscillations in cataclysmic variables and X-Ray binaries. In addition to the earlier recognition that both types possess the same correlation between high and low frequency quasi-periodic…

天体物理学 · 物理学 2009-11-10 Brian Warner , Patrick A. Woudt

A model to explain variable gamma-ray sources with high-mass microblazars is described. Inverse Compton interactions between the jet of a microquasar and the UV-photon field of the stellar companion can produce high-energy gamma-rays. The…

天体物理学 · 物理学 2007-05-23 M. M. Kaufman Bernado , G. E. Romero , I. F. Mirabel

High-mass microquasars are binary systems consisting of a massive star and an accreting compact object from which relativistic jets are launched. There is considerable observational evidence that winds of massive stars are clumpy.…

高能天体物理现象 · 物理学 2015-05-13 Anabella T. Araudo , Valenti Bosch-Ramon , Gustavo E. Romero

We performed simultaneous observations in 3 bands (UBV) of the flickering variability of the recurrent novae RS Oph and T CrB at quiescence. Using new and published data, we compare the colours of the flickering in cataclysmic variables and…

太阳与恒星天体物理 · 物理学 2015-06-23 R. Zamanov , S. Boeva , G. Latev , K. A. Stoyanov , S. V. Tsvetkova

An inclusive search is performed for supersymmetry in final states containing jets and an apparent imbalance in transverse momentum, pt[miss], due to the production of unobserved weakly interacting particles in pp collisions at a…

高能物理 - 实验 · 物理学 2017-02-28 CMS Collaboration

Hard-scattered partons provide an ideal probe for the study of the Quark-Gluon Plasma because they are produced prior to the formation of the QCD medium in heavy-ion collisions. Jet production is therefore susceptible to modifications…

核实验 · 物理学 2019-08-13 Salvatore Aiola

Time-resolved optical and infrared polarimetric observations of black hole and neutron star low-mass X-ray binaries are presented. Data were acquired with the VLT, UKIRT and HIPPO on the SAAO 1.9-m. We find that for some sources in…

AG Draconis produces a strong supersoft X-ray emission.The X-ray and optical/UV fluxes are in a strict anticorrelation throughout the active and quiescent phases. The aim of this contribution is to identify the source of the X-ray emission…

高能天体物理现象 · 物理学 2015-05-13 A. Skopal , M. Sekeras , R. Gonzalez-Riestra , R. F. Viotti

The properties of jets produced in p+p, d+Au and Au+Au collisions at sqrt{s_NN}=200 GeV are studied using the method of two particle correlations. The trigger particle is assumed to be a leading particle from a high p_T jet while the…

高能物理 - 实验 · 物理学 2009-11-10 Jan Rak

In heavy-ion collisions, nuclear matter is subjected to extreme conditions in a highly dynamical, rapidly evolving environment. This poses a tremendous challenge for calculating jet quenching observables. Current approaches rely on…

高能物理 - 唯象学 · 物理学 2026-05-29 Souvik Priyam Adhya , Konrad Tywoniuk

Several observations of stellar jets show evidence of X-ray emitting shocks close to the launching site. In some cases, the shocked features appear to be stationary, also for YSOs at different stages of evolution. We study the case of HH…

太阳与恒星天体物理 · 物理学 2018-08-01 S. Ustamujic , S. Orlando , R. Bonito , M. Miceli , A. I. Gómez de Castro

SS433 is well-known for its precessing twin jets having optical bullets inferred through {\it spectroscopic} observation of $H_\alpha$ lines. Recently, Chakrabarti et al. (2002) described processes which may be operating in accretion disk…

天体物理学 · 物理学 2009-11-10 Sandip K. Chakrabarti , S. Pal , A. Nandi , B. G. Anandarao , Soumen Mondal

A search for supersymmetry in final states with jets and missing transverse energy is performed in pp collisions at a centre-of-mass energy of sqrt(s) = 7 TeV. The data sample corresponds to an integrated luminosity of 4.98 inverse…

高能物理 - 实验 · 物理学 2014-03-12 CMS Collaboration

To probe the properties of the quark-gluon plasma created in heavy-ion collisions, a very useful class of observables refers to the propagation of energetic jets. A jet is a collimated spray of particles generated via successive parton…

高能物理 - 唯象学 · 物理学 2020-10-07 Paul Caucal

Collisions of heavy ion nuclei at relativistic speeds (close to the speed of light) creates a high temperature and very dense form of matter, now known to consist of de-confined quarks and gluons, named the quark gluon plasma (QGP). In this…

高能物理 - 实验 · 物理学 2018-03-13 Raghav Kunnawalkam Elayavalli

We study the modifications of jets created in heavy-ion collisions at LHC energies. The inherent hierarchy of scales governing the jet evolution allows to distinguish a leading jet structure, which interacts coherently with the medium as a…

高能物理 - 唯象学 · 物理学 2015-07-15 Yacine Mehtar-Tani , Konrad Tywoniuk
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