Zobrazeno 1 - 10
of 153
pro vyhledávání: '"Jerome Rodriguez"'
Autor:
Constanza Echiburú-Trujillo, Alexandra J. Tetarenko, Daryl Haggard, Thomas D. Russell, Karri I. I. Koljonen, Arash Bahramian, Jingyi Wang, Michael Bremer, Joe Bright, Piergiorgio Casella, David M. Russell, Diego Altamirano, M. Cristina Baglio, Tomaso Belloni, Chiara Ceccobello, Stephane Corbel, Maria Diaz Trigo, Dipankar Maitra, Aldrin Gabuya, Elena Gallo, Sebastian Heinz, Jeroen Homan, Erin Kara, Elmar Körding, Fraser Lewis, Matteo Lucchini, Sera Markoff, Simone Migliari, James C. A. Miller-Jones, Jerome Rodriguez, Payaswini Saikia, Craig L. Sarazin, Tariq Shahbaz, Gregory Sivakoff, Roberto Soria, Vincenzo Testa, Bailey E. Tetarenko, Valeriu Tudose
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 2, p 116 (2024)
Black hole (BH) X-ray binaries (XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multiwavelength observations of the Galactic BH system MAXI J1820+070, throughout its 2018
Externí odkaz:
https://doaj.org/article/494f93ddc0a741aa8d221ca3efa1875d
Autor:
Susmita Chakravorty, Pierre-Olivier Petrucci, Sudeb Ranjan Datta, Jonathan Ferreira, Joern Wilms, Jonatan Jacquemin-Ide, Maica Clavel, Gregoire Marcel, Jerome Rodriguez, Julien Malzac, Renaud Belmont, Stephane Corbel, Mickael Coriat, Gilles Henri, Maxime Parra
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 518 (1), pp.1335-1351. ⟨10.1093/mnras/stac2835⟩
Monthly Notices of the Royal Astronomical Society, 2023, 518 (1), pp.1335-1351. ⟨10.1093/mnras/stac2835⟩
In our self-similar, analytical, magneto-hydrodynamic (MHD) accretion-ejection solution, the density at the base of the outflow is explicitly dependent on the disk accretion rate - a unique property of this class of solutions. We had earlier found th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c465aa09aba44718223a0acd4fd5d338
http://arxiv.org/abs/2209.15127
http://arxiv.org/abs/2209.15127
Autor:
Arash Bodaghee, Aarran W. Shaw, Francesca M. Fornasini, Sylvain Chaty, Jeremy Hare, John A. Tomsick, Roman Krivonos, Maïca Clavel, Jerome Rodriguez, Benjamin M. Coughenour
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2021, 914 (1), pp.48. ⟨10.3847/1538-4357/abfa1a⟩
Astrophys.J.
Astrophys.J., 2021, 914 (1), pp.48. ⟨10.3847/1538-4357/abfa1a⟩
The Astrophysical Journal, American Astronomical Society, 2021, 914 (1), pp.48. ⟨10.3847/1538-4357/abfa1a⟩
Astrophys.J.
Astrophys.J., 2021, 914 (1), pp.48. ⟨10.3847/1538-4357/abfa1a⟩
Here we report on X-ray observations of ten 17-60 keV sources discovered by the INTEGRAL satellite. The primary new information is sub-arcsecond positions obtained by the Chandra X-ray Observatory. In six cases (IGR J17040-4305, IGR J18017-3542, IGR
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35a021da3212dc75c9b1b29d6dbfcf0d
Autor:
Francesca M. Fornasini, Maïca Clavel, Sylvain Chaty, Roman Krivonos, Jerome Rodriguez, Jeremy Hare, John A. Tomsick, Arash Bodaghee, Farid Rahoui
Publikováno v:
Astrophys.J.
Astrophys.J., 2020, 889 (1), pp.53. ⟨10.3847/1538-4357/ab5fd2⟩
Astrophys.J., 2020, 889 (1), pp.53. ⟨10.3847/1538-4357/ab5fd2⟩
The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) satellite has detected in excess of 1000 sources in the ~20-100 keV band during its surveys of the sky over the past 17 years. We obtained 5 ks observations of 15 unclassified IGR sources
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28510a62d8a21752ef9cabe4c18e120e
https://hal.archives-ouvertes.fr/hal-02467271
https://hal.archives-ouvertes.fr/hal-02467271
Autor:
Hung-Hsiang Liang, Yi-Chi Chang, Hsiang-Yue, Jerome Rodriguez, Jeng-Lun Chiu, Chien-Ying Yang, Philippe Laurent, Che-Yen Chu, Chih-Hsun Lin, Hsiang-Kuang Chang
Publikováno v:
Astron.J.
Astron.J., 2020, 160 (1), pp.54. ⟨10.3847/1538-3881/ab9caf⟩
Astron.J., 2020, 160 (1), pp.54. ⟨10.3847/1538-3881/ab9caf⟩
Instruments flown on CubeSats are small. Meaningful applications of CubeSats in astronomical observations rely on the choice of a particular subject that is feasible for CubeSats. Here we report the result of a feasibility study for observing gamma-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c39abedd5ea2124796b99fe7c39c6446
https://hal.science/hal-02416913
https://hal.science/hal-02416913
Autor:
Brenton Jackson, Jerome Rodriguez, Andreas Zezas, Arash Bodaghee, Vallia Antoniou, Eric Frechette, Ryan Agnew, Zachary Jordan, Ann Hornschemeier, John A. Tomsick
Publikováno v:
Astrophys.J.
Astrophys.J., 2021, 919 (2), pp.81. ⟨10.3847/1538-4357/ac11f4⟩
Astrophys.J., 2021, 919 (2), pp.81. ⟨10.3847/1538-4357/ac11f4⟩
We present the two-point cross-correlation function between high-mass X-ray binaries (HMXBs) in the Small Magellanic Cloud (SMC) and their likely birthplaces (OB Associations: OBAs). This function compares the spatial correlation between the observed
Autor:
ShuangNan Zhang, Andrea Santangelo, Marco Feroci, YuPeng Xu, FangJun Lu, Yong Chen, Hua Feng, Shu Zhang, Søren Brandt, Margarita Hernanz, Luca Baldini, Enrico Bozzo, Riccardo Campana, Alessandra De Rosa, YongWei Dong, Yuri Evangelista, Vladimir Karas, Norbert Meidinger, Aline Meuris, Kirpal Nandra, Teng Pan, Giovanni Pareschi, Piotr Orleanski, QiuShi Huang, Stephane Schanne, Giorgia Sironi, Daniele Spiga, Jiri Svoboda, Gianpiero Tagliaferri, Christoph Tenzer, Andrea Vacchi, Silvia Zane, Dave Walton, ZhanShan Wang, Berend Winter, Xin Wu, Jean J. M. in’ t Zand, Mahdi Ahangarianabhari, Giovanni Ambrosi, Filippo Ambrosino, Marco Barbera, Stefano Basso, Jörg Bayer, Ronaldo Bellazzini, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Giacomo Borghi, XueLei Cao, Franck Cadoux, Francesco Ceraudo, TianXiang Chen, YuPeng Chen, Jerome Chevenez, Marta Civitani, Wei Cui, WeiWei Cui, Thomas Dauser, Ettore Del Monte, Sergio Di Cosimo, Sebastian Diebold, Victor Doroshenko, Michal Dovciak, YuanYuan Du, Lorenzo Ducci, QingMei Fan, Yannick Favre, Fabio Fuschino, José Luis Gálvez, Min Gao, MingYu Ge, Olivier Gevin, Marco Grassi, QuanYing Gu, YuDong Gu, DaWei Han, Bin Hong, Wei Hu, Long Ji, ShuMei Jia, WeiChun Jiang, Thomas Kennedy, Ingo Kreykenbohm, Irfan Kuvvetli, Claudio Labanti, Luca Latronico, Gang Li, MaoShun Li, Xian Li, Wei Li, ZhengWei Li, Olivier Limousin, HongWei Liu, XiaoJing Liu, Bo Lu, Tao Luo, Daniele Macera, Piero Malcovati, Adrian Martindale, Malgorzata Michalska, Bin Meng, Massimo Minuti, Alfredo Morbidini, Fabio Muleri, Stephane Paltani, Emanuele Perinati, Antonino Picciotto, Claudio Piemonte, JinLu Qu, Alexandre Rachevski, Irina Rashevskaya, Jerome Rodriguez, Thomas Schanz, ZhengXiang Shen, LiZhi Sheng, JiangBo Song, LiMing Song, Carmelo Sgro, Liang Sun, Ying Tan, Phil Uttley, Bo Wang, DianLong Wang, GuoFeng Wang, Juan Wang, LangPing Wang, YuSa Wang, Anna L. Watts, XiangYang Wen, Jörn Wilms, ShaoLin Xiong, JiaWei Yang, Sheng Yang, YanJi Yang, Nian Yu, WenDa Zhang, Gianluigi Zampa, Nicola Zampa, Andrzej A. Zdziarski, AiMei Zhang, ChengMo Zhang, Fan Zhang, Long Zhang, Tong Zhang, Yi Zhang, XiaoLi Zhang, ZiLiang Zhang, BaoSheng Zhao, ShiJie Zheng, YuPeng Zhou, Nicola Zorzi, J. Frans Zwart
Publikováno v:
Science China Physics, Mechanics & Astronomy
ResearcherID
Sci.China Phys.Mech.Astron.
Sci.China Phys.Mech.Astron., 2019, 62 (2), pp.29502. ⟨10.1007/s11433-018-9309-2⟩
Science China: Physics, Mechanics and Astronomy, 62(2):29502. Science in China Press
ResearcherID
Sci.China Phys.Mech.Astron.
Sci.China Phys.Mech.Astron., 2019, 62 (2), pp.29502. ⟨10.1007/s11433-018-9309-2⟩
Science China: Physics, Mechanics and Astronomy, 62(2):29502. Science in China Press
In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::41fa2f15a34a13e97b0ac3397a3c3527
http://hdl.handle.net/20.500.12386/30599
http://hdl.handle.net/20.500.12386/30599
Autor:
R. Belmont, Julien Malzac, Maïca Clavel, S. Chakravorty, Stephane Corbel, G. Henri, Jonathan Ferreira, Jerome Rodriguez, S. Drappeau, Mickael Coriat, P.-O. Petrucci
Publikováno v:
Astronomische Nachrichten. 337:429-434
We want to test if self-similar magneto-hydrodynamic (MHD) accretion-ejection models can explain the observational results for accretion disk winds in BHBs. In our models, the density at the base of the outflow from the accretion disk is not a free p
Publikováno v:
Astronomische Nachrichten. 337:435-440
Black hole X-ray binaries display large outbursts, during which their properties are strongly variable. We develop a sys¬tematic spectral analysis of the 3–40 keV RXTE/PCA data in order to study the evolution of these systems and apply it to GX 33
Autor:
Piergiorgio Casella, Jeroen Homan, John A. Tomsick, Jerome Rodriguez, T. M. Belloni, Sara Motta, M. Cadolle Bel, Victoria Grinberg, B. Sbarufatti, Emrah Kalemci, M. Del Santo, A. J. Castro-Tirado, Katja Pottschmidt, Jörn Wilms, T. Muñoz-Darias, Stephane Corbel
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 456:3585-3595
We studied time variability and spectral evolution of the Galactic black hole transient Swift J174510.8-262411 during the first phase of its outburst. INTEGRAL and Swift observations collected from 2012 September 16 until October 30 have been used. T