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The origin of Galactic cosmic rays remains a matter of debate, but supernova remnants are commonly considered to be the main place where high-energy cosmic rays are accelerated. Nevertheless, current models predict cosmic-ray spectra that…

High Energy Astrophysical Phenomena · Physics 2021-06-23 G. J. Escobar , L. J. Pellizza , G. E. Romero

We present a model for high-energy emission in microquasars where the energy content of the jets is dominated by relativistic protons. We also include a primary leptonic component. Particles are accelerated up to relativistic energies in a…

Astrophysics · Physics 2009-11-13 Gabriela S. Vila , Gustavo E. Romero

Collimated outflows (jets) appear to be a ubiquitous phenomenon associated with the accretion of material onto a compact object. Despite this ubiquity, many fundamental physics aspects of jets are still poorly understood and constrained.…

High Energy Astrophysical Phenomena · Physics 2017-02-15 Gustavo Romero , Markus Boettcher , Sera Markoff , Fabrizio Tavecchio

We propose that relativistic Galactic jets like those observed in GRS 1915+105 and GRO J1655-40 may produce small but measurable contributions to the cosmic ray (CR) spectrum. If these jets contain cold protons and heavy ions (as in SS433),…

Astrophysics · Physics 2009-11-07 S. Heinz , R. A. Sunyaev

Microquasar (MQ) jets are sites of particle acceleration and synchrotron emission. Such synchrotron radiation has been detected coming from jet regions of different spatial scales, which for the instruments at work nowadays appear as…

Astrophysics · Physics 2008-11-26 V. Bosch-Ramon

A population of unidentified gamma-ray sources is forming a structure resembling a halo around the Galactic center. These sources are highly variable, and hence they should be associated with compact objects. Microquasars are objects…

Astrophysics · Physics 2008-07-02 Gustavo E. Romero , Gabriela S. Vila

Jets are ubiquitous in the Universe. They are collimated outflows whose origin is associated to an accretion disc and a central object, and can be very powerful non-thermal emitters. Jets form in active galactic nuclei, gamma-ray bursts,…

High Energy Astrophysical Phenomena · Physics 2015-05-30 V. Bosch-Ramon

I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena and astroparticle physics. After reminding…

Astrophysics · Physics 2007-05-23 Sylvain Chaty

Microquasars are compact binary systems hosting collimated relativistic jets. They have long been proposed as cosmic-ray accelerators, probed via the gamma-ray emission produced by relativistic particles. However, the observational evidence…

High Energy Astrophysical Phenomena · Physics 2024-10-15 G. Martí-Devesa , L. Olivera-Nieto

I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena. After remindind the analogy with quasars,…

Astrophysics · Physics 2007-05-23 Sylvain Chaty

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced in star formation regions in distant galaxies by highly relativistic jets that happen to point in our direction. Relativistic beaming collimates the…

Astrophysics · Physics 2007-05-23 Arnon Dar

The origin of Galactic cosmic rays (CRs), particularly around the knee region ($\sim$3 PeV), remains a major unsolved question. Recent observations by LHAAASO suggest that the knee is shaped mainly by protons, with a transition to heavier…

High Energy Astrophysical Phenomena · Physics 2025-12-09 B. Theodore Zhang , Shigeo S. Kimura , Kohta Murase

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.…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Anabella T. Araudo , Valenti Bosch-Ramon , Gustavo E. Romero

Microquasars such as SS 433 are considered potential contributors to cosmic rays up to the knee of the cosmic ray energy spectrum ($\sim4\,\mathrm{PeV}$), where a transition in the dominant acceleration processes is expected. The SS 433…

To some extent, all Galactic binary systems hosting a compact object are potential `microquasars', so much as all galactic nuclei may have been quasars, once upon a time. The necessary ingredients for a compact object of stellar mass to…

High Energy Astrophysical Phenomena · Physics 2014-11-20 E. Gallo

Observational and theoretical studies point to microquasars (MQs) as possible counterparts of a significant fraction of the unidentified gamma-ray sources detected so far. At present, a proper scenario to explain the emission beyond soft…

Astrophysics · Physics 2009-11-11 V. Bosch-Ramon , G. E. Romero , J. M. Paredes

Suppose that even the highest energy cosmic rays (CRs) observed on Earth are protons accelerated in local Milky Way Galaxy sources, with few if any from more distant sources. In this paper we treat the problem that supernovae remnants…

High Energy Astrophysical Phenomena · Physics 2013-05-06 Richard Shurtleff

The jets associated with Galactic micro-quasars are believed to be ejected by accreting stellar mass black-holes or neutron stars. We show that if the energy content of the jets in the transient sources is dominated by electron-proton…

High Energy Physics - Phenomenology · Physics 2009-11-07 Amir Levinson , Eli Waxman

I review recent progress in the theory of relativistic jet production. The presently favored mechanism is an electrodynamic one, in which charged plasma is accelerated by electric fields that are generated by a rotating magnetic field. The…

Astrophysics · Physics 2007-05-23 David L. Meier

Core-collapse supernovae are found in galaxies with ongoing star-formation. In a starburst galaxy hosting an active galactic nucleus with a relativistic jet, supernovae can take place inside the jet. The collision of the supernova ejecta…

High Energy Astrophysical Phenomena · Physics 2019-02-20 F. L. Vieyro , V. Bosch-Ramon , N. Torres-Albà
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