F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, A. R. Bazer‐Bachi, B. Behera, M. Beilicke, W. Benbow, D. Berge, K. Bernlöhr, C. Boisson, O. Bolz, V. Borrel, I. Braun, E. Brion, J. Brucker, R. Bühler, T. Bulik, I. Büsching, T. Boutelier, S. Carrigan, P. M. Chadwick, L.‐M. Chounet, A. C. Clapson, G. Coignet, R. Cornils, L. Costamante, M. Dalton, B. Degrange, H. J. Dickinson, A. Djannati-Ataı̈, W. Domainko, L. O’C. Drury, F. Dubois, G. Dubus, J. Dyks, K. Egberts, D. Emmanoulopoulos, P. Espigat, C. Farnier, F. Feinstein, A. Fiaßon, A. Förster, G. Fontaine, M. Füßling, Y. A. Gallant, B. Giebels, J. F. Glicenstein, B. Glück, P. Goret, C. Hadjichristidis, D. Hauser, M. Häuser, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, A. Hoffmann, W. Hofmann, M. Holleran, S. Hoppe, D. Horns, A. Jachołkowska, O. C. de Jager, I. Jung, K. Katarzyński, E. Kendziorra, M. Kerschhaggl, B. Khélifi, D. Keogh, Nu. Komin, K. Kosack, G. Lamanna, I. J. Latham, M. Lemoine‐Goumard, J.-P. Lenain, T. Lohse, Jean‐Michel Martin, O. Martineau‐Huynh, A. Marcowith, C. Masterson, D. Maurin, T. J. L. McComb, R. Moderski, E. Moulin, M. Naumann-Godó, M. de Naurois, D. Nedbal, D. Nekrassov, S. J. Nolan, S. Ohm, J.-P. Olive, E. de Oña Wilhelmi, K. J. Orford, J. L. Osborne, M. Ostrowski, M. Panter, G. Pedaletti, G. Pelletier, P.‐O. Petrucci, S. Pita, G. Pühlhofer, M. Punch, A. Quirrenbach, Britt Raubenheimer, M. Raue, S. M. Rayner, M. Renaud, J. Ripken, L. Rob, S. Rosier-Lees, Gavin Rowell, B. Rudak, J. Ruppel, V. Sahakian, A. Santangelo, R. Schlickeiser, F. M. Schöck, R. Schröder, U. Schwanke, S. Schwarzburg, S. Schwemmer, A. Shalchi, H. Sol, D. Spangler, Ł. Stawarz, R. Steenkamp, C. Stegmann, G. Superina, P. H. T. Tam, J.‐P. Tavernet, R. Terrier, C. van Eldik, G. Vasileiadis, C. Venter, J. P. Vialle, P. Vincent, M. Vivier, H. J. Völk, F. Volpe, S. J. Wagner, M. J. Ward, A. A. Zdziarski, A. Zech,
Aims. Observations of Kepler's supernova remnant (G4.5+6.8) with the HESS telescope array in 2004 and 2005 with a total live time of 13 h are presented.
Tópico(s): Astrophysical Phenomena and Observations
2008 - EDP Sciences | Astronomy and Astrophysics
A. De Angelis, selenia broccio,
A supernova close enough to the Earth is a spectacular event: it can appear as a “new star” as luminous as Venus, or even more, visible for several days. The rate of Galactic supernovae is expected to be of about one in 30 years, with a fraction visible to the naked eye; however in all the history of human civilization only seven supernovae in the Milky Way have been reported, the last two (1572 and 1604) during Galilei’s life. The supernova of 1604, today called Kepler’s Supernova, was observed by ...
Tópico(s): Astrophysical Phenomena and Observations
2021 - Multidisciplinary Digital Publishing Institute | Universe
Kepler's interpretation of the supernova of 1604, De Stella Nova, interwove the science of astronomy with astrology and theology in an attempt to determine ...
Tópico(s): Historical Astronomy and Related Studies
2009 - Nature Portfolio | Nature
Isamu Hatsukade, H. Tsunemi, Koujun Yamashita, Katsuji Koyama, Yoshihiro Asaoka, Ikuko Asaoka,
... dans l'intervalle 1-12 keV, du reste de supernova Kepler (SN 1604) sont presentees. Le spectre RX est analyse. Une forte raie d'emission Kα de fer a 6.48 keV est determinee. Les ...
Tópico(s): Astronomy and Astrophysical Research
1990 - Oxford University Press | Publications of the Astronomical Society of Japan
A scenario for the origin of Kepler's supernova remnant is presented. According to this scenario the progenitor was a massive runaway star, subject to strong mass loss. Due to the interaction of the wind with the interstellar medium, a bow shock has formed in the direction of the stellar motion. Using the available data on the remnant, various constraints on the progenitor's wind can be set. A search has been carried out, among classes of known runaway objects to determine the nature of the progenitor. ...
Tópico(s): Spaceflight effects on biology
1988 - Springer Nature (Netherlands) | Astrophysics and space science library
F. Aharonian, F. Ait Benkhali, E. O. Angüner, Halim Ashkar, Michael Backes, V. Barbosa Martins, R. Batzofin, Y. Becherini, D. Berge, K. Bernlöhr, M. Böttcher, C. Boisson, J. Bolmont, Mathieu de Bony de Lavergne, M. Breuhaus, Robert Brose, F. Brun, T. Bulik, T. Bylund, F. Cangemi, Sami Caroff, S. Casanova, M. Cerruti, T. Chand, A. Chen, O. Chibueze, G. Cotter, Pierre Cristofari, J. Damascene Mbarubucyeye, J. Devin, A. Djannati-Ataı̈, A. Dmytriiev, K. Egberts, S. Einecke, J.-P. Ernenwein, Kirsty Feijen, A. Fiaßon, G. Fichet de Clairfontaine, G. Fontaine, S. Funk, S. Gabici, Y. A. Gallant, S. Ghafourizadeh, G. Giavitto, Luca Giunti, D. Glawion, J. F. Glicenstein, M.-H. Grondin, M. Hörbe, Werner Hofmann, T. L. Holch, M. Holler, D. Horns, Zhi-Qiu Huang, M. Jamrozy, V. Joshi, I. Jung-Richardt, E. Kasai, K. Katarzyński, U. Katz, B. Khélifi, W. Kluźniak, Nu. Komin, K. Kosack, D. Kostunin, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, Fabian Leuschner, T. Lohse, A. Luashvili, I. Lypova, Jonathan Mackey, D. Malyshev, D. Malyshev, V. Marandon, ¶. Marchegiani, A. Marcowith, G. Martí-Devesa, R. Marx, G. Maurin, P. J. Meintjes, M. Meyer, Alison Mitchell, R. Moderski, L. Mohrmann, A. Montanari, E. Moulin, J. Muller, K. Nakashima, M. de Naurois, A. Nayerhoda, J. Niemiec, A. Priyana Noel, P. O’Brien, S. Ohm, Laura Olivera-Nieto, E. de Ona Wilhelmi, M. Ostrowski, Sebastian Panny, M. Panter, R. D. Parsons, Giada Peron, V. Poireau, D. A. Prokhorov, G. Pühlhofer, M. Punch, A. Quirrenbach, Patrick Reichherzer, O. Reimer, O. Reimer, M. Renaud, Brian Reville, Frank Rieger, Gavin Rowell, B. Rudak, H. Rueda Ricarte, V. Sahakian, S. Sailer, D. A. Sanchez⋆, D. A. Sanchez⋆, A. Santangelo, M. Sasaki, J. S. Schafer, F. Schüßler, Hester Schutte, U. Schwanke, J. N. S. Shapopi, R. Simoni, H. Sol, A. Specovius, S. Spencer, Ł. Stawarz, S. Steinmassl, Constantin Steppa, I. Sushch, T. Takahashi, T. Tanaka, A. M. Taylor, R. Terrier, M. Tsirou, Y. Uchiyama, T. Unbehaun, C. van Eldik, J. Veh, Jacco Vink, H. J. Völk, S. J. Wagner, Felix Werner, R. White, A. Wierzcholska, Yu Wun Wong, A. Yusafzai, M. Zacharias, D. Zargaryan, A. A. Zdziarski, A. Zech, S. J. Zhu, S. Zouari, N. Żywucka,
Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of nearby supernova (SN) remnants with ages younger than 500 yr by establishing Cassiopeia A and the remnant of Tycho’s SN as very-high-energy (VHE) γ -ray sources. The remnant of Kepler’s SN, which is the product of the most recent naked-eye SN in our Galaxy, is comparable in age to the other two, but is significantly more distant. If the γ -ray luminosities of the remnants of Tycho’s and Kepler’s SNe are ...
Tópico(s): Dark Matter and Cosmic Phenomena
2022 - EDP Sciences | Astronomy and Astrophysics
The fluid dynamical model of Gull (1973a, b) predicts that the radio emission of young supernova remnants occurs in instabilities at the boundary between the ejected mass and the 'swept-up' interstellar medium, and that no central energy source is necessary. High resolution radio observations of the thickness, polarization properties and structure of the shells of such objects provide a test for these theories, and also enable an upper limit to be set on the flux from point sources within the shell ...
Tópico(s): Radio Astronomy Observations and Technology
1974 - Springer Nature (Netherlands) | Astrophysics and space science library
... émissivité. Les résultats obtenus sur les Supernovae de Képler et Tycho Brahé sont en accord avec ceux de Cal Tech sur 960 Mc/s: la Supernova de Tycho Brahé est peut-être une enveloppe sphérique, mais on ne peut rien dire de celle de Képler.
Tópico(s): Astronomy and Astrophysical Research
1964 - Cambridge University Press | Symposium - International Astronomical Union
F. Aharonian, F. Ait Benkhali, E. O. Angüner, Halim Ashkar, Michael Backes, V. Barbosa Martins, R. Batzofin, Y. Becherini, D. Berge, K. Bernlöhr, M. Böttcher, C. Boisson, J. Bolmont, M. de Bony de Lavergne, M. Breuhaus, R. Brose, F. Brun, T. Bulik, T. Bylund, F. Cangemi, Sami Caroff, S. Casanova, M. Cerruti, T. Chand, A. Chen, O. Chibueze, G. Cotter, P. I. Cristofari, J. Damascene Mbarubucyeye, J. Devin, A. Djannati-Ataï, A. Dmytriiev, K. Egberts, S. Einecke, J.-P. Ernenwein, Kirsty Feijen, A. Fiasson, G. Fichet de Clairfontaine, G. Fontaine, S. Funk, S. Gabici, Y. A. Gallant, S. Ghafourizadeh, G. Giavitto, Luca Giunti, D. Glawion, J. F. Glicenstein, M.-H. Grondin, M. Hörbe, W. Hofmann, T. L. Holch, M. Holler, D. Horns, Zhiqiu Huang, M. Jamrozy, V. Joshi, I. Jung-Richardt, E. Kasai, K. Katarzyński, U. Katz, B. Khélifi, W. Kluźniak, Nu. Komin, K. Kosack, D. Kostunin, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, Fabian Leuschner, T. Lohse, Anna Luashvili, I. Lypova, Jonathan Mackey, D. Malyshev, D. Malyshev, V. Marandon, ¶. Marchegiani, Alexandre Marcowith, G. Martí-Devesa, R. Marx, G. Maurin, P. J. Meintjes, M. Meyer, Alison Mitchell, R. Moderski, L. Mohrmann, A. Montanari, E. Moulin, J. Muller, K. Nakashima, M. de Naurois, A. Nayerhoda, J. Niemiec, A. Priyana Noel, P. O’Brien, S. Ohm, Laura Olivera-Nieto, E. de Ona Wilhelmi, M. Ostrowski, Sebastian Panny, M. Panter, R. D. Parsons, Giada Peron, V. Poireau, D. A. Prokhorov, G. Pühlhofer, M. Punch, A. Quirrenbach, Patrick Reichherzer, A. Reimer, O. Reimer, M. Renaud, Brian Reville, Frank Rieger, G. Rowell, B. Rudak, H. Rueda Ricarte, V. Sahakian, S. Sailer, H. Salzmann, D. A. Sanchez⋆, A. Santangelo, M. Sasaki, J. S. Schafer, F. Schüßler, Hester Schutte, U. Schwanke, J. N. S. Shapopi, R. Simoni, H. Sol, A. Specovius, S. Spencer, Ł. Stawarz, S. Steinmassl, C. Steppa, I. Sushch, T. Takahashi, T. Tanaka, A. M. Taylor, R. Terrier, M. Tsirou, Y. Uchiyama, T. Unbehaun, C. van Eldik, J. Veh, J. Vink, H. J. Völk, S. J. Wagner, F. Werner, R. White, A. Wierzcholska, Yu Wun Wong, A. Yusafzai, M. Zacharias, D. Zargaryan, A. A. Zdziarski, A. Zech, S. J. Zhu, S. Zouari, N. Żywucka,
N 0 = (9.5 ± 2.3 stat ± 2.9 sys ) × 10 -14 cm -2 s -1 TeV -1 .The normalization was correctly stated elsewhere.
Tópico(s): Dark Matter and Cosmic Phenomena
2024 - EDP Sciences | Astronomy and Astrophysics
... detail, writing an entire book on his observations, De Stella Nova in Pede Serpentarii (On the New Star in Ophiuchus's Foot). His book contained an original drawing of the position of the stars with the shadow of Ophiuchus framing the constellation. new star appears in the heel of the constellation, labeled 'N'. As result of this work, SN1604 is now also known as Kepler's Supernova. supernova and Kepler's methodical observations of planted ...
Tópico(s): Healthcare, Law, Governance, and Management Studies
2012 - Taylor & Francis | Research-Technology Management
Produção Nacional
Revisado por pares
Wenxiong Li, Xiaofeng Wang, J. Vinkó, J. Mo, G. Hosseinzadeh, David J. Sand, Jujia Zhang, H. Lin, Jujia Zhang, Lingzhi Wang, Jujia Zhang, Zhihao Chen, Danfeng Xiang, L. Rui, Fan Huang, Xue Li, Xiaodan Zhang, L. Li, E. Baron, James M. DerKacy, Xulin Zhao, H. Sai, Kaicheng Zhang, Lingzhi Wang, D. A. Howell, C. McCully, I. Arcavi, S. Valenti, D. Hiramatsu, J. Burke, A. Rest, P. Garnavich, B. Tucker, Gautham Narayan, E. Shaya, S. Margheim, A. Zenteno, V. Ashley Villar, G. Dimitriadis, R. J. Foley, Y. C. Pan, D. A. Coulter, Ori D. Fox, Saurabh W. Jha, D. O. Jones, Daniel Kasen, C. D. Kilpatrick, Anthony L. Piro, Adam G. Riess, C. Rojas-Bravo, B. J. Shappee, T. W. S. Holoien, K. Z. Stanek, M. R. Drout, Katie Auchettl, C. S. Kochanek, J. S. Brown, S. Bose, D. Bersier, J. Brimacombe, Ping Chen, Subo Dong, S. Holmbo, J. A. Muñoz, R. L. Mutel, R. S. Post, J. L. Prieto, J. Shields, D. Tallon, Todd A. Thompson, P. Vallely, Steven Villanueva, S. J. Smartt, K. W. Smith, K. C. Chambers, H. Flewelling, M. E. Huber, E. A. Magnier, C. Waters, A. S. B. Schultz, J. Bulger, T. Lowe, M. Willman, K. Sárneczky, András Pál, J. C. Wheeler, Attila Bódi, Zsófia Bognár, B. Csák, B. Cseh, G. Csörnyei, O. Hanyecz, Bernadett Ignácz, Csilla Kalup, Réka Könyves-Tóth, L. Kriskovics, A. Ordasi, I. Rajmon, Á. Sódor, R. Szabó, R. Szakáts, Gabriella Zsidi, Peter Milne, Jennifer E. Andrews, Nathan Smith, Christopher Bilinski, P. J. Brown, J. Nordin, S. C. Williams, L. Galbany, J. Palmerio, I. Hook, C. Inserra, K. Maguire, R. Cartier, Alessandro Razza, C. P. Gutiérrez, J. J. Hermes, Joshua S. Reding, Benjamin C. Kaiser, J. Tonry, A. Heinze, L. Denneau, H. Weiland, B. Stalder, Geert Barentsen, Jessie L. Dotson, Thomas Barclay, Michael Gully-Santiago, Christina Hedges, Ann Marie Cody, Steve B. Howell, Jeffrey L. Coughlin, Jeffrey E. Van Cleve, Josè Vinícius de Miranda Cardoso, K. A. Larson, K. M. McCalmont-Everton, C. Peterson, S. Ross, Lee Reedy, Darren Osborne, Chris McGinn, L. Kohnert, Lucas F. Migliorini, A. Wheaton, Brittany Spencer, C. Labonde, G. A. Rodrıguez Castillo, G. Beerman, K. Steward, M. Hanley, R. Larsen, R. Gangopadhyay, R. Kloetzel, T. Weschler, V. Nystrom, J. Moffatt, M. Redick, K. Griest, M. Packard, M. Muszynski, Jennifer Kampmeier, R. Bjella, S. Flynn, B. Elsaesser,
... 18bt) is the first spectroscopically confirmed Type Ia supernova (SN Ia) observed in the Kepler field. The Kepler data revealed an excess emission ...
Tópico(s): Astrophysics and Cosmic Phenomena
2018 - IOP Publishing | The Astrophysical Journal
Produção Nacional
Revisado por pares
G. Dimitriadis, R. J. Foley, A. Rest, Daniel Kasen, Anthony L. Piro, Abigail Polin, D. O. Jones, A. Villar, Gautham Narayan, D. A. Coulter, C. D. Kilpatrick, Y. C. Pan, C. Rojas-Bravo, Ori D. Fox, Saurabh W. Jha, P. Nugent, Adam G. Riess, D. Scolnic, M. R. Drout, Geert Barentsen, Jessie L. Dotson, Michael Gully-Santiago, Christina Hedges, Ann Marie Cody, Thomas Barclay, Steve B. Howell, P. Garnavich, B. Tucker, E. Shaya, R. F. Mushotzky, R. Olling, S. Margheim, A. Zenteno, Jeffrey L. Coughlin, Jeffrey E. Van Cleve, Josè Vinícius de Miranda Cardoso, K. A. Larson, K. M. McCalmont-Everton, C. Peterson, S. Ross, Lee Reedy, Darren Osborne, Chris McGinn, L. Kohnert, Lucas F. Migliorini, A. Wheaton, Brittany Spencer, C. Labonde, G. A. Rodrıguez Castillo, G. Beerman, K. Steward, M. Hanley, R. Larsen, R. Gangopadhyay, R. Kloetzel, T. Weschler, V. Nystrom, J. Moffatt, M. Redick, K. Griest, M. Packard, M. Muszynski, Jennifer Kampmeier, R. Bjella, S. Flynn, B. Elsaesser, K. C. Chambers, H. Flewelling, M. E. Huber, E. A. Magnier, C. Waters, A. S. B. Schultz, J. Bulger, T. Lowe, M. Willman, S. J. Smartt, K. Smith, Sean Points, G. Strampelli, J. Brimacombe, Ping Chen, J. A. Muñoz, R. L. Mutel, J. Shields, P. Vallely, Steven Villanueva, Wenxiong Li, Lingzhi Wang, Jujia Zhang, H. Lin, J. Mo, Xulin Zhao, H. Sai, Xiaodan Zhang, Kaicheng Zhang, Jujia Zhang, Lingzhi Wang, Jujia Zhang, E. Baron, James M. DerKacy, L. Li, Zhihao Chen, Danfeng Xiang, L. Rui, Lingzhi Wang, Fang Huang, Xue Li, G. Hosseinzadeh, D. A. Howell, I. Arcavi, D. Hiramatsu, J. Burke, S. Valenti, J. Tonry, L. Denneau, A. Heinze, H. Weiland, B. Stalder, J. Vinkó, K. Sárneczky, András Pál, Attila Bódi, Zs. Bognár, B. Csák, B. Cseh, G. Csörnyei, O. Hanyecz, Bernadett Ignácz, Csilla Kalup, Réka Könyves-Tóth, L. Kriskovics, A. Ordasi, I. Rajmon, Á. Sódor, R. Szabó, R. Szakáts, Gabriella Zsidi, S. C. Williams, J. Nordin, R. Cartier, C. Frohmaier, L. Galbany, C. P. Gutiérrez, I. Hook, C. Inserra, M. Smith, David J. Sand, Jennifer E. Andrews, Nathan Smith, Christopher Bilinski,
We present an exquisite, 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt), starting weeks before explosion, covering the moment of explosion and the subsequent rise, and continuing past peak brightness. ...
Tópico(s): Pulsars and Gravitational Waves Research
2018 - IOP Publishing | The Astrophysical Journal Letters
... Magellanic Cloud was not only the brightest since Keplers supernova in 1604, but also the very first supernova in history which could be studied in ...
Tópico(s): Neutrino Physics Research
1989 - Springer Nature | Reviews in modern astronomy
David A. Green, F. R. Stephenson,
... accounts include the well-recorded supernovae of AD1604 (Kepler's SN), AD1572 (Tycho's SN), AD1181 AD1054 (which produced the Crab Nebula) and AD1006, together with less certain events dating back to AD185. In the case of the supernovae of AD1604 and AD1572 it is European records that provide the most accurate information available, whereas for earlier supernovae records are principally from East Asian sources. Also discussed briefly are several spurious supernova candidates, and the future prospects for studies of ...
Tópico(s): Astrophysics and Cosmic Phenomena
2003 - Springer Science+Business Media | Lecture notes in physics
... of astronomy have, understandably, centred on luminaries like Kepler and Galileo to see how objects like the supernova of 1604 cracked the crystalline purity of the ...
Tópico(s): Historical Studies on Spain
2015 - SAGE Publishing | Journal for the History of Astronomy
... in the Large Magellanic Cloud was the brightest supernova since the one sighted by Kepler in 1604. There have been remarkable improvements in ...
Tópico(s): Stellar, planetary, and galactic studies
1991 - Cambridge University Press | Transactions of the International Astronomical Union
A number of young supernova remnants (SNRs) are now known to have nonthermal X-ray spectra. The steepness of the X-ray emission suggests that it is synchrotron from TeV electrons, and if this is the case, efficient shock acceleration is likely occurring in these objects. Here we use a model of nonlinear diffusive shock acceleration to fit the broad-band emission from SN1006, Tycho’s, and Kepler’s SNRs. Our fits confirm that all of these SNRs are producing TeV particles, but also show that the electron ...
Tópico(s): Neutrino Physics Research
2001 - Springer Nature (Netherlands) | Space sciences series of ISSI
A. Decourchelle, Donald C. Ellison,
... how efficient particle acceleration modifies the dynamics of supernova remnants, and use the X-ray spectral data on Kepler’s remnant to illustrate the effects on the ...
Tópico(s): Astrophysical Phenomena and Observations
2001 - Springer Nature (Netherlands) | Space sciences series of ISSI
... rapporte la detection et la cartographie de Tycho, Kepler et CasA dans la bande 10-100 μm. ...
Tópico(s): Astronomy and Astrophysical Research
1987 - EDP Sciences | Astronomy and Astrophysics
Hideo Matsufuru, Kohsuke Sumiyoshi,
... performance is examined on two systems with the Kepler and Pascal generations of NVIDIA’s GPU architecture.
Tópico(s): Gamma-ray bursts and supernovae
2018 - Springer Science+Business Media | Lecture notes in computer science
... the Crab. The remnant of Tycho Brahe’s supernova of 1572 is that of a typical SN Ia. The SNRs of SN 1006 and that seen by Johannes Kepler in 1604 are virtually certain remnants of SN ...
Tópico(s): Pulsars and Gravitational Waves Research
2017 - Springer International Publishing | Astronomy and astrophysics library
A number of young supernova remnants (SNRs) are now known to have nonthermal X-ray spectra. The steepness of the X-ray emission suggests that it is synchrotron from TeV electrons, and if this is the case, efficient shock acceleration is likely occurring in these objects. Here we use a model of nonlinear diffusive shock acceleration to fit the broad-band emission from SN1006, Tycho's, and Kepler's SNRs. Our fits confirm that all of these SNRs are producing TeV particles, but also show that the electron ...
Tópico(s): Astrophysical Phenomena and Observations
2001 - Springer Nature (Netherlands) | Astrophysics and space science library
... magnetic fields are seen in Galactic objects like supernova remnants, in radio galaxies or even in the ...
Tópico(s): Gamma-ray bursts and supernovae
2023 - Springer International Publishing | Historical & cultural astronomy
... ceux de 3 autres restes de supernovae, Tycho, Kepler, et Cas A.
Tópico(s): Astronomy and Astrophysical Research
1990 - EDP Sciences | Astronomy and Astrophysics