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Related papers: Ellerman bombs: fallacies, fads, usage

200 papers

The blazar 3C 279 is well known for its prolific emission of rapid flares. A particular event occurred on 12/20/2013, exhibiting a large flux increase with a doubling time scale of a few hours, a very hard gamma-ray spectrum, and a…

High Energy Astrophysical Phenomena · Physics 2025-01-27 Sébastien Le Bihan , Anton Dmytriiev , Andreas Zech

Lyman alpha blobs - luminous, spatially extended emission-line nebulae, often lacking bright continuum counterparts - are common in dense environments at high redshift. Until recently, atmospheric absorption and filter technology have…

Astrophysics of Galaxies · Physics 2015-05-13 William C. Keel , Raymond E. White III. , Scott Chapman , Rogier A. Windhorst

Blazars are the most violent steady/recurrent sources of high-energy gamma-ray emission in the known Universe. They are prominent emitters of electromagnetic radiation throughout the entire electromagnetic spectrum. The observable radiation…

Astrophysics · Physics 2008-11-26 Markus Boettcher

Recent gamma-ray burst observations have revealed late-time, highly energetic events which deviate from the simplest expectations of the standard fireball picture. Instead they may indicate that the central engine is active or restarted at…

Astrophysics · Physics 2009-11-13 Andrew King , Paul T. O'Brien , Michael R. Goad , Julian Osborne , Emma Olsson , Kim Page

We analyze optical spectra of a two-ribbon, long duration C1.1 flare that occurred on 18 Aug 2011 within AR 11271 (SOL2011-08-18T15:15). The impulsive phase of the flare was observed with a comprehensive set of space-borne and ground-based…

Solar and Stellar Astrophysics · Physics 2015-06-23 Adam F. Kowalski , Gianna Cauzzi , Lyndsay Fletcher

UV bursts and Ellerman bombs are transient brightenings observed in the low solar atmospheres of emerging flux regions. Observations have discovered the cospatial and cotemporal EBs and UV bursts, and their formation mechanisms are still…

Solar and Stellar Astrophysics · Physics 2021-02-17 Lei Ni , Yajie Chen , Hardi Peter , Hui Tian , Jun Lin

D. Wouters and P. Brun in Phys. Rev. D 86, 043005 (2012) claim that an observable effect in the spectra of distant very-high-energy blazars arises as a consequence of oscillations of photons into axion-like particles (ALPs) in the presence…

High Energy Astrophysical Phenomena · Physics 2013-06-27 Giorgio Galanti , Marco Roncadelli

Strongly intermittent turbulence is observed in the shadow of a limiter in the Large Plasma Device (LAPD) at UCLA [W. Gekelman, H. Pfister, Z. Lucky, J. Bamber, D. Leneman, and J. Maggs, Rev. Sci. Inst. {\bfseries 62}, 2875 (1991)]. The…

Plasma Physics · Physics 2009-11-11 T. A. Carter

There are two goals in this study. One is to investigate how frequently white-light flares (WLFs) occur in a flare-productive active region (NOAA active region 11515). The other is to investigate the relationship between WLFs and magnetic…

Solar and Stellar Astrophysics · Physics 2018-06-06 Y. L. Song , H. Tian , M. Zhang , M. D. Ding

Blazars, a unique class of active galactic nuclei, exhibit highly variable emission across the electromagnetic spectrum. This variability frequently manifests as intense flaring events, sparking an ongoing debate in recent literature about…

High Energy Astrophysical Phenomena · Physics 2025-04-08 Pablo Peñil , Nuria Torres-Albà , Alba Rico , Marco Ajello , Sara Buson , Sagar Adhikari

Intergalactic magnetic fields (IGMF) can cause the appearance of halos around the gamma-ray images of distant objects because an electromagnetic cascade initiated by a high-energy gamma-ray interaction with the photon background is…

High Energy Astrophysical Phenomena · Physics 2015-03-17 Shin'ichiro Ando , Alexander Kusenko

Ultra-long Gamma-Ray Bursts are a class of high energy transients lasting several hours. Their exact nature is still elusive, and several models have been proposed to explain them. Because of the limited coverage of wide field gamma-ray…

High Energy Astrophysical Phenomena · Physics 2019-06-03 B. Gendre , Q. T. Joyce , N. B. Orange , G. Stratta , J. L. Atteia , M. Boer

The ideas of topology have found tremendous success in Hermitian physical systems, but even richer properties exist in the more general non-Hermitian framework. Here, we theoretically propose and experimentally demonstrate a new…

(abridged) Non-ionizing stellar continua are a source of photons for continuum pumping in the hydrogen Lyman transitions. In the environments where these transitions are optically thick, deexcitation occurs through higher series lines, so…

In this work we investigate the properties of the broad emission line components in the Balmer series of a sample of Type 1 Active Galactic Nuclei (AGN). Using the Boltzmann Plot method as a diagnostic tool for physical conditions in the…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 G. La Mura , F. Di Mille , L. Č. Popović , S. Ciroi , P. Rafanelli , D. Ilić

This paper summarizes the observations which provide the best evidence for the presence of black holes in active galactic nuclei. This includes: X-ray variability; kinematical studies using optical emission lines as well as the distribution…

Astrophysics · Physics 2007-05-23 Greg M. Madejski

Gamma-ray bursts are sudden releases of energy that for a duration of a few seconds outshine even huge galaxies. 30 years after the first detection of a gamma-ray burst their origin remains a mystery. Here I first review the ``old''…

Astrophysics · Physics 2007-05-23 Jochen Greiner

The gamma ray burst phenomenon is reviewed from a theoretical point of view, with emphasis on the fireball shock scenario of the prompt emission and the longer wavelenght afterglow. Recent progress and issues are discussed, including…

Astrophysics · Physics 2009-11-07 P. Meszaros

Coalescing binary systems, consisting of two collapsed objects, are among the most promising sources of high frequency gravitational waves signals detectable, in principle, by ground-based interferometers. Binary systems of Neutron Star or…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-16 S. Capozziello , M. De Laurentis , I. De Martino , M. Formisano

We compute the polarization of the Lyman alpha line photons emerging from an anisotropically expanding and optically thick medium, which is expected to operate in many Lyman alpha emitting objects including the primeval galaxy DLA~2233+131…

Astrophysics · Physics 2009-10-30 Hee-Won Lee , Sang-Hyeon Ahn
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