English
Related papers

Related papers: SS 433: flares in H alpha, GRAVITY observations & …

200 papers

Gamma-ray burst X-ray flares are believed to mark the late time activity of the central engine. We compute the temporal evolution of the average flare luminosity $< L >$ in the common rest frame energy band of 44 GRBs taken from the large…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. Margutti , G. Bernardini , R. Barniol Duran , C. Guidorzi , R. F. Shen , G. Chincarini

SS 433 is a microquasar whose relativistic jets precess every ~162 days, providing a laboratory for jet-interstellar medium interactions. We present a comprehensive analysis of 16 years of Fermi Large Area Telescope data (August…

High Energy Astrophysical Phenomena · Physics 2026-05-18 Ömer Faruk Çoban , Diego F. Torres , Jian Li , Daniela Hadasch , Agnibha De Sarkar , Matthew Kerr

We present multiwavelength data for twelve blazars observed from 2008-2010 as part of an ongoing optical-infrared photometric monitoring project. Sources were selected to be bright, southern (dec < 20 deg) blazars observed by the Fermi…

High Energy Astrophysical Phenomena · Physics 2015-06-03 E. W. Bonning , C. M. Urry , C. Bailyn , M. Buxton , R. Chatterjee , P. Coppi , G. Fossati , J. Isler , L. Maraschi

Solar spicules are chromospheric fibrils that appear everywhere on the Sun, yet their origin is not understood. Using high resolution observations of spicules obtained with the Swedish 1-m Solar Telescope, we aim to understand how spicules…

Solar and Stellar Astrophysics · Physics 2016-06-22 Tiago M. D. Pereira , Luc Rouppe van der Voort , Mats Carlsson

Blazars, a subclass of active galactic nuclei (AGN), are known to be bright $\gamma$-ray sources, frequently exhibiting active (flaring) periods. The blazar PKS~2155-304 is a high synchrotron-peaked BL Lac object located at redshift…

High Energy Astrophysical Phenomena · Physics 2024-02-26 Hong-Bin Tan , Ruo-Yu Liu , Markus Böttcher

We have performed 5 night spectroscopic observation of the Halpha line of EV Lac with a medium wavelength resolution (R~ 10,000) using the 2m Nayuta telescope at the Nishi-Harima Astronomical Observatory. EV Lac always possesses the Halpha…

Solar and Stellar Astrophysics · Physics 2018-05-30 Satoshi Honda , Yuta Notsu , Kosuke Namekata , Shota Notsu , Hiroyuki Maehara , Kai Ikuta , Daisaku Nogami , Kazunari Shibata

This paper presents the multi-wavelength analysis of a 13 s quasi-periodic pulsation (QPP) observed in hard X-ray (12-300 keV) and microwave (4.9-34 GHz) emissions during a C-class flare occurred on 21 September 2015. AIA 304 and 171 \AA~…

Solar and Stellar Astrophysics · Physics 2017-02-22 Pankaj Kumar , Valery M. Nakariakov , Kyung-Suk Cho

We have investigated the dipping activity observed in the high-mass X-ray binary 4U 1907+09 and shown that the source continues to pulsate in the "off" state, noting that the transition between the "on" and "off" states may be either…

High Energy Astrophysical Phenomena · Physics 2012-10-17 V. Doroshenko , A. Santangelo , L. Ducci , D. Klochkov

Several redback and black widow millisecond pulsar binaries have episodes of flaring in X-rays and optical. We initially detected such behavior from the Fermi selected redback candidate 1FGL J0523.5$-$2529 during optical time-series…

High Energy Astrophysical Phenomena · Physics 2022-08-31 Jules P. Halpern , Karen I. Perez , Slavko Bogdanov

Recurrent flaring events at X- and soft gamma-ray energies have been recently reported for the galactic black hole candidate Cygnus X-1. The observed fluxes during these transient outbursts are far higher than what is observed in ``normal''…

Astrophysics · Physics 2009-11-07 G. E. Romero , M. M. Kaufman Bernado , I. F. Mirabel

The extreme space weather conditions resulting from high energetic events likes solar flares and Coronal Mass Ejections (CMEs) demand for reliable space weather forecasting. The magnetic flux tubes while rising through the convection zone…

Solar and Stellar Astrophysics · Physics 2022-10-19 B Lekshmi , Kiran Jain , Rudolf W. Komm , Dibyendu Nandy

We report simultaneous X-ray and infrared (IR) observations of the Galactic microquasar GRS1915+105 using XTE and the Palomar 200-inch telescope on August 13-15, 1997 UTC. During the last two nights, the microquasar GRS 1915+105 exhibited…

Astrophysics · Physics 2009-10-30 S. S. Eikenberry , K. Matthews , E. H. Morgan , R. A. Remillard , R. W. Nelson

After 33 years of extensive studies of SS 433, we have learnt much about this unique system with moving emission lines in the spectrum. The orbital inclination is known from spectroscopic observations of moving lines; the distance is…

High Energy Astrophysical Phenomena · Physics 2011-10-26 V. P. Goranskij

We discuss the results of the radio studies of the X-ray binaries with relativistic jets. We carried out a multi-frequency (1-30 GHz) daily monitoring of the radio flux variability of the microquasars SS433, GRS1915+105, and Cyg X-3 with…

Astrophysics · Physics 2009-06-25 Sergei A. Trushkin , Nikolaj A. Nizhelskij , Nikolaj N. Bursov

Blazars are a subclass of radio-loud active galactic nuclei (AGNs), where the jet is aligned close to the line of sight. Blazars emission is dominated by non-thermal processes, where Doppler boosted radiation originates from a relativistic…

High Energy Astrophysical Phenomena · Physics 2021-08-19 Jakub Juryšek , Vitalii Sliusar , Dimitri Moulin , Roland Walter

The GRAVITY interferometer has achieved microarcsecond precision in near-infrared interferometry, enabling the tracking of flare centroid motion in the strong gravitational field near the Sgr A*. It might be promising to serve as a unique…

High Energy Astrophysical Phenomena · Physics 2026-01-09 Fengting Xie , Qing-Hua Zhu , Xin Li

Context. Blazar AO 0235+164, located at redshift z = 0.94, has undergone several sharp multi-spectral-range flaring episodes during the last decades. In particular, the episodes peaking in 2008 and 2015, that received extensive…

The blazar PKS 0903-57 has recently been classified as a flat spectrum radio quasar at a redshift of $z=0.2621$. In March and April 2020, Fermi-LAT and AGILE reported tremendous activity in high-energy $\gamma$ rays with the flux increasing…

High Energy Astrophysical Phenomena · Physics 2026-03-16 A. Acharyya , F. Aharonian , F. Ait Benkhali , A. Alkan , H. Ashkar , M. Backes , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , K. Bernlöhr , B. Bi , M. Böttcher , C. Boisson , J. Bolmont , J. Borowska , R. Brose , A. Brown , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Casanova , J. Celic , M. Cerruti , S. Chandra , A. Chen , M. Chernyakova , J. O. Chibueze , O. Chibueze , B. Cornejo , G. Cotter , G. Cozzolongo , J. Damascene Mbarubucyeye , J. de Assis Scarpin , M. de Naurois , E. de Oña Wilhelmi , A. G. Delgado Giler , J. Devin , A. Djannati-Ataï , J. Djuvsland , A. Dmytriiev , V. Doroshenko , K. Egg , S. Einecke , J. -P. Ernenwein , C. Escañuela Nieves , K. Feijen , M. D. Filipovic , G. Fontaine , S. Funk , S. Gabici , Y. A. Gallant , M. Genaro , J. F. Glicenstein , P. Goswami , G. Grolleron , L. Haerer , L. Heckmann , G. Hermann , B. Heß , J. A. Hinton , W. Hofmann , T. L. Holch , M. Holler , D. Horns , M. Jamrozy , F. Jankowsky , I. Jung-Richardt , E. Kasai , K. Katarzyński , D. Kerszberg , R. Khatoon , B. Khélifi , W. Kluźniak , N. Komin , D. Kostunin , R. G. Lang , A. Lemièr , J. -P. Lenain , A. Luashvili , J. Mackey , D. Malyshev , V. Marandon , G. Martí-Devesa , R. Marx , M. Mayer , A. Mehta , A. M. W. Mitchell , R. Moderski , M. O. Moghadam , L. Mohrmann , A. Montanari , E. Moulin , D. Moyeni , J. Niemiec , L. Olivera-Nieto , S. Panny , M. Panter , R. D. Parsons , U. Pensec , S. Pita , G. Pühlhofer , A. Quirrenbach , M. Regeard , A. Reimer , O. Reimer , H. X. Ren , B. Reville , F. Rieger , G. Rowell , B. Rudaka , K. Sabri , V. Sahakiana , H. Salzmann , M. Sasaki , J. Schäfer , F. Schüssler , H. M. Schutte , J. N. S. Shapopi , A. Sharma , W. Si Said , H. Sol , S. Spencer , Ł. Stawarz , R. Steenkamp , S. Steinmassl , C. Steppa , T. Takahashi , T. Tanaka , A. M. Taylor , C. van Eldik , M. Vecchi , J. Vink , T. Wach , S. J. Wagner , A. Wierzcholska , M. Zacharias , A. A. Zdziarski , A. Zech , N. Żywucka

GRS 1915+105 has exhibited at least three modes of long-wavelength (infrared to radio) flares. Class A flares are the bright ($\sim 1$ Jy) radio events whose apparent superluminal motion in many ways defines the microquasars. Class B flares…

Astrophysics · Physics 2007-05-23 Stephen Eikenberry

Multi-wavelength monitoring of Sgr A* flaring activity confirms the presence of embedded structures within the disk on size scales commensurate with the innermost accretion region, matching size scales that are derived from observed light…

High Energy Astrophysical Phenomena · Physics 2015-11-10 E M Howard
‹ Prev 1 8 9 10 Next ›