Zobrazeno 1 - 10 of 210 pro vyhledávání: '"F. Mirabel"'
1
Report
The prompt, high resolution spectroscopic view of the 'naked-eye' GRB080319B
Autor: D'Elia, V., Fiore, F., Perna, R., Krongold, Y., Covino, S., Fugazza, D., Lazzati, D., Nicastro, F., Antonelli, L. A., Campana, S., Chincarini, G., D'Avanzo, P., Della Valle, M., Goldoni, P., Guetta, D., Guidorzi, C., Meurs, E. J. A., Molinari, F. Mirabel E., Norci, L., Piranomonte, S., Stella, L., Stratta, G., Tagliaferri, G., Ward, P.
Publikováno v: Astrophys.J.694:332-338,2009
GRB080319B reached 5th optical magnitude during the burst prompt emission. Thanks to the VLT/UVES rapid response mode, we observed its afterglow just 8m:30s after the GRB onset when the magnitude was R ~ 12. This allowed us to obtain the best signal-
Externí odkaz: http://arxiv.org/abs/0804.2141
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2
Akademický článek
A strainmeter array as the fulcrum of novel observatory sites along the Alto Tiberina Near Fault Observatory
Autor: L. Chiaraluce, R. Bennett, D. Mencin, W. Johnson, M. R. Barchi, M. Bohnhoff, P. Baccheschi, A. Caracausi, C. Calamita, A. Cavaliere, A. Gualandi, E. Mandler, M. T. Mariucci, L. Martelli, S. Marzorati, P. Montone, D. Pantaleo, S. Pucci, E. Serpelloni, M. Supino, S. Stramondo, C. Hanagan, L. Van Boskirk, M. Gottlieb, G. Mattioli, M. Urbani, F. Mirabella, A. Akimbekova, S. Pierdominici, T. Wiersberg, C. Marone, L. Palmieri, L. Schenato
Publikováno v: Scientific Drilling, Vol 33, Pp 173-190 (2024)
Fault slip is a complex natural phenomenon involving multiple spatiotemporal scales from seconds to days to weeks. To understand the physical and chemical processes responsible for the full fault slip spectrum, a multidisciplinary approach is highly
Externí odkaz: https://doaj.org/article/7928bd577f9d435b817dd13e35ea6bd9
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3
Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
Autor: I. F. Mirabel
Publikováno v: IAU Symp.
IAU Symposium 346
IAU Symposium 346, Aug 2018, Vienna, Austria. pp.365-379, ⟨10.1017/S1743921319002084⟩
Theoretical models and observations suggest that primordial Stellar Black Holes (Pop-III-BHs) were prolifically formed in HMXBs, which are powerful relativistic jet sources of synchrotron radiation called Microquasars (MQs). Large populations of BH-H
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6f05084cabf16b01c39f83c22dcf51f
https://hal.archives-ouvertes.fr/hal-02024217
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4
Black holes formed by direct collapse: observational evidences
Autor: I. F. Mirabel
Publikováno v: IAU Symp.
IAU Symposium 324
IAU Symposium 324, Sep 2016, Ljubljana, Slovenia. IAU Symp., 324, pp.303-306, 2016, 〈10.1017/S1743921316012904〉
IAU Symposium 324, Sep 2016, Ljubljana, Slovenia. pp.303-306, ⟨10.1017/S1743921316012904⟩
Binary black holes as the recently detected sources of gravitational waves can be formed from massive stellar binaries in the field or by dynamical interactions in clusters of high stellar density, if the black holes are the remnants of massive stars
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23d21dcc8382534b28acd6ea5049f295
https://hal.archives-ouvertes.fr/hal-01584669
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5
Stellar progenitors of black holes: insights from optical and infrared observations
Autor: I. F. Mirabel
Publikováno v: IAU Symp.
IAU Symposium 324
IAU Symposium 324, Sep 2016, Ljubljana, Slovenia. IAU Symp., 324, pp.27-30, 2016, 〈10.1017/S1743921316012576〉
IAU Symposium 324, Sep 2016, Ljubljana, Slovenia. pp.27-30, ⟨10.1017/S1743921316012576⟩
Here are reviewed the insights from observations at optical and infrared wavelengths for low mass limits above which stars do not seem to end as luminous supernovae. These insights are: (1) the absence in archived images of nearby galaxies of stellar
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a311655c9f05caf35f632af2f7dde079
https://hal.archives-ouvertes.fr/hal-01584668
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6
The e-ASTROGAM gamma-ray space mission
Autor: Andrei M. Bykov, A. De Angelis, Dieter H. Hartmann, Sheila McBreen, Uwe Oberlack, M. Cardillo, C. Pittori, D. Bernard, Sandro Mereghetti, Francesco Longo, Philippe Laurent, Jürgen Knödlseder, R. Walter, Andreas Zoglauer, Valentina Fioretti, Marco Tavani, S. Sabatini, A. Brogna, Martino Marisaldi, C. Labanti, Jordi Isern, Kazuhiro Nakazawa, J. Peyré, Paolo Coppi, Julie McEnery, A. Morselli, J. Kiener, Lorraine Hanlon, G. Piano, Andrzej A. Zdziarski, Xin Wu, A. Argan, Andrea Bulgarelli, Riccardo Campana, D. J. Thompson, P. A. Caraveo, Margarita Hernanz, Alessio Aboudan, P. von Ballmoos, F. Mirabel, I. Donnarumma, V. Tatischeff, I. A. Grenier, Olivier Limousin, G. Kanbach, Roland Diehl, Alexei Ulyanov, J. E. Grove, L. Stawarz, A. Giuliani, C. Hamadache
Publikováno v: Proc.SPIE Int.Soc.Opt.Eng.
Space Telescopes and Instrumentation 2016
Space Telescopes and Instrumentation 2016, Jun 2016, Edinburgh, United Kingdom. pp.99052N, ⟨10.1117/12.2231601⟩
NASA Astrophysics Data System
Space Telescopes and Instrumentation 2016, Jun 2016, Edinburgh, United Kingdom. Proc.SPIE Int.Soc.Opt.Eng., 9905, pp.99052N, 2016, 〈10.1117/12.2231601〉
Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
The e-ASTROGAM is a gamma-ray space mission to be proposed as the M5 Medium-size mission of the European Space Agency. It is dedicated to the observation of the Universe with unprecedented sensitivity in the energy range 0.2 - 100 MeV, extending up t
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4fd5225404d5a4b890b4a004bb82084
https://hal.archives-ouvertes.fr/hal-01554037
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7
Enhanced X-ray emission from Lyman Break Analogues and a Possible $L_{\rm X}$--SFR--Metallicity Plane
Autor: Philip Kaaret, I. F. Mirabel, M. Brorby, Andrea Prestwich
Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The source of energetic photons that heated and reionized the early Universe remains uncertain. Early galaxies had low metallicity and recent population synthesis calculations suggest that the number and luminosity of high-mass X-ray binaries are enh
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ff629e07072a764969389f8f86ce16b
http://arxiv.org/abs/1602.01091
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8
Morphology and Molecular Gas Fractions of Local Luminous Infrared Galaxies as a Function of Infrared Luminosity and Merger Stage
Autor: K. L. Larson, D. B. Sanders, J. E. Barnes, C. M. Ishida, A. S. Evans, V. U, J. M. Mazzarella, D.-C. Kim, G. C. Privon, I. F. Mirabel, H. A. Flewelling
Publikováno v: Astrophys.J.
Astrophys.J., 2016, 825 (2), pp.128. ⟨10.3847/0004-637X/825/2/128⟩
We present a new, detailed analysis of the morphologies and molecular gas fractions (MGFs) for a complete sample of 65 local luminous infrared galaxies from Great Observatories All-Sky Luminous Infrared Galaxies (LIRG) Survey using high resolution I-
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cdf3f725a1f895845a50df1f55f30140
https://hal.archives-ouvertes.fr/hal-01554974
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9
THE OPTICAL AND NEAR-INFRARED COUNTERPART OF GRS 1758-258
Autor: I. F. Mirabel, Josep Martí, Juan R. Sánchez-Sutil, Pedro L. Luque-Escamilla, A. J. Muñoz-Arjonilla, Jorge Ariel Combi, E. Sánchez-Ayaso
Publikováno v: International Journal of Modern Physics D. 19:757-761
GRS 1758-258 is one of the two brightest persistent hard X–ray sources in the Galactic Center region, of which an optical/near infrared counterpart has not been unambiguously identified in previous work, mainly due to high absorption and the lack o
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::9a89b2b0be42be4440d031aea792c43f
https://doi.org/10.1142/s0218271810016725
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