Search Results - "ISM: supernova remnants"

Characterizing mass, momentum, energy, and metal outflow rates of multiphase galactic winds in the FIRE-2 cosmological simulations by Pandya, Viraj, Fielding, Drummond B, Anglés-Alcázar, Daniel, Somerville, Rachel S, Bryan, Greg L, Hayward, Christopher C, Stern, Jonathan, Kim, Chang-Goo, Quataert, Eliot, Forbes, John C, Faucher-Giguère, Claude-André, Feldmann, Robert, Hafen, Zachary, Hopkins, Philip F, Kereš, Dušan, Murray, Norman, Wetzel, Andrew

“…ABSTRACT We characterize mass, momentum, energy, and metal outflow rates of multiphase galactic winds in a suite of FIRE-2 cosmological ‘zoom-in’ simulations…”
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A diagnostic tool for the identification of supernova remnants by Kopsacheili, M, Zezas, A, Leonidaki, I

“…We present new diagnostic tools for distinguishing supernova remnants (SNRs) from H ii regions. Up to now, sources with flux ratio [S ii]/H$\rm {\alpha }$…”
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Evolution of supernovae-driven superbubbles with conduction and cooling by El-Badry, Kareem, Ostriker, Eve C, Kim, Chang-Goo, Quataert, Eliot, Weisz, Daniel R

“…We use spherically symmetric hydrodynamic simulations to study the dynamical evolution and internal structure of superbubbles (SBs) driven by clustered…”
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The infancy of core-collapse supernova remnants by Gabler, Michael, Wongwathanarat, Annop, Janka, Hans-Thomas

“…ABSTRACT We present 3D hydrodynamic simulations of neutrino-driven supernovae (SNe) with the Prometheus-HotB code, evolving the asymmetrically expanding ejecta…”
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The gas-to-extinction ratio and the gas distribution in the Galaxy by Zhu, Hui, Tian, Wenwu, Li, Aigen, Zhang, Mengfei

“…Abstract We investigate the relation between the optical extinction (A V ) and the hydrogen column density (N H) determined from X-ray observations of a large…”
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Revisiting the dust destruction efficiency of supernovae by Priestley, F D, Chawner, H, Matsuura, M, De Looze, I, Barlow, M J, Gomez, H L

“…ABSTRACT Dust destruction by supernovae is one of the main processes removing dust from the interstellar medium (ISM). Estimates of the efficiency of this…”
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The morphology of the ejecta of SN 1987A at 31 yr from 1150 to 10 000 angstrom by Kangas, Tuomas, Fransson, C., Larsson, Josefin, France, K., Chevalier, R. A., Kirshner, R. P., Lundqvist, P., Mattila, S., Sollerman, J., Utrobin, V. P.

“…We present spectroscopy of the ejecta of SN 1987A in 2017 and 2018 from the Hubble Space Telescope and the Very Large Telescope, covering the wavelength range…”
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A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A by Ahnen, M. L., Ansoldi, S., Arcaro, C., Babić, A., Bangale, P., Barres de Almeida, U., Becerra González, J., Bednarek, W., Bernardini, E., Berti, A., Biasuzzi, B., Biland, A., Blanch, O., Bonnoli, G., Carosi, R., Chatterjee, A., Colin, P., Colombo, E., Contreras, J. L., Cumani, P., Da Vela, P., Dazzi, F., De Angelis, A., de Oña Wilhelmi, E., Dominis Prester, D., Dorner, D., Eisenacher Glawion, D., Elsaesser, D., Engelkemeier, M., Fallah Ramazani, V., Fernández-Barral, A., Fidalgo, D., Font, L., Fruck, C., Galindo, D., Garczarczyk, M., Gaug, M., Giammaria, P., Godinović, N., Gora, D., Guberman, D., Hadasch, D., Hahn, A., Hassan, T., Hayashida, M., Herrera, J., Hose, J., Hrupec, D., Konno, Y., Kubo, H., Kushida, J., Kuveždić, D., Lelas, D., Maggio, C., Makariev, M., Maneva, G., Manganaro, M., Maraschi, L., Mariotti, M., Martínez, M., Minev, M., Mirzoyan, R., Moreno, V., Moretti, E., Neustroev, V., Niedzwiecki, A., Nilsson, K., Nishijima, K., Noda, K., Nogués, L., Paiano, S., Palacio, J., Paoletti, R., Paredes, J. M., Perri, L., Prada Moroni, P. G., Puljak, I., Garcia, J. R., Reichardt, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Satalecka, K., Schweizer, T., Shore, S. N., Stamerra, A., Strzys, M., Surić, T., Tavecchio, F., Temnikov, P., Terzić, T., Tescaro, D., Teshima, M., Torres-Albà, N., Treves, A., Vanzo, G., Vovk, I., Ward, J. E., Zarić, D.

“…Abstract It is widely believed that the bulk of the Galactic cosmic rays is accelerated in supernova remnants (SNRs). However, no observational evidence of the…”
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The distribution of radioactive $^{44}$Ti in Cassiopeia A by Grefenstette, Brian W., Fryer, Chris L., Harrison, Fiona A., Boggs, Steven E., Delaney, Tracey, Laming, J. Martin, Reynolds, Stephen P., Alexander, David M., Barret, Didier, Christensen, Finn E., Craig, William W., Forster, Karl, Giommi, Paolo, Hailey, Charles J., Hornstrup, Alan, Kitaguchi, Takao, Koglin, J.E., Lopez, Laura, Mao, Peter H., Madsen, Kristin K., Miyasaka, Hiromasa, Mori, Kaya, Perri, Matteo, Pivovaroff, Michael J., Puccetti, Simonetta, Rana, Vikram, Stern, Daniel, Westergaard, Niels J., Wik, Daniel R., Zhang, William W., Zoglauer, Andreas

“…The distribution of elements produced in the innermost layers of a supernova explosion is a key diagnostic for studying the collapse of massive stars. Here we…”
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Thermal and kinematic properties of ejecta in SN1987A revealed by XRISM by Audard, Marc, Awaki, Hisamitsu, Ballhausen, Ralf, Bamba, Aya, Behar, Ehud, Boissay-Malaquin, Rozenn, Brown, Gregory V, Costantini, Elisa, Cumbee, Renata, Díaz Trigo, María, Dotani, Tadayasu, Ebisawa, Ken, Enoto, Teruaki, Ezoe, Yuichiro, Foster, Adam, Fukazawa, Yasushi, Furuzawa, Akihiro, Gallo, Luigi C, Gu, Liyi, Guainazzi, Matteo, Giuffrida, Roberta, Hagino, Kouichi, Hatsukade, Isamu, Hayashi, Katsuhiro, Hell, Natalie, Hodges-Kluck, Edmund, Hornschemeier, Ann, Ichinohe, Yuto, Ishi, Daiki, Ishida, Manabu, Ishisaki, Yoshitaka, Kallman, Timothy, Kikuchi, Ryunosuke, Kilbourne, Caroline, Kobayashi, Shogo, Loewenstein, Michael, Maeda, Yoshitomo, Markevitch, Maxim, Matsumoto, Hironori, McCammon, Dan, McNamara, Brian, Miller, Eric D, Mitsuishi, Ikuyuki, Mizumoto, Misaki, Mizuno, Tsunefumi, Mori, Koji, Mukai, Koji, Murakami, Hiroshi, Nakazawa, Kazuhiro, Nobukawa, Kumiko, Nobukawa, Masayoshi, Noda, Hirofumi, Ogawa, Shoji, Ogorzalek, Anna, Okajima, Takashi, Ota, Naomi, Paltani, Stephane, Petre, Robert, Porter, Frederick Scott, Pottschmidt, Katja, Sato, Kosuke, Sato, Toshiki, Sawada, Makoto, Seta, Hiromi, Shidatsu, Megumi, Shimoda, Jiro, Suzuki, Hiromasa, Szymkowiak, Andrew, Takahashi, Hiromitsu, Takeo, Mai, Tamagawa, Toru, Tamura, Keisuke, Tanimoto, Atsushi, Tashiro, Makoto, Terada, Yukikatsu, Terashima, Yuichi, Tsuboi, Yohko, Tsujimoto, Masahiro, Tsunemi, Hiroshi, Tsuru, Takeshi Go, Uchida, Hiroyuki, Uchida, Nagomi, Uchida, Yuusuke, Uchiyama, Hideki, Ueda, Shutaro, Ueda, Yoshihiro, Uno, Shinichiro, Watanabe, Shin, Williams, Brian J, Yamada, Satoshi, Yamada, Shinya, Yamaguchi, Hiroya, Yamasaki, Noriko, Yamauchi, Makoto, Yamauchi, Shigeo, Yoneyama, Tomokage, Yukita, Mihoko, Zhuravleva, Irina, Miceli, Marco, Sapienza, Vincenzo

“…Abstract We present an analysis of high-resolution spectra from the shock-heated plasmas in SN 1987A, based on an observation using the Resolve instrument…”
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Exotic baryons in hot neutron stars by Issifu, A, Marquez, K D, Pelicer, M R, Menezes, D P

“…ABSTRACT We study the nuclear isentropic equation of state for a stellar matter composed of nucleons, hyperons, and Δ-resonances. We investigate different…”
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The momentum budget of clustered supernova feedback in a 3D, magnetized medium by Gentry, Eric S, Krumholz, Mark R, Madau, Piero, Lupi, Alessandro

“…While the evolution of superbubbles driven by clustered supernovae has been studied by numerous authors, the resulting radial momentum yield is uncertain by as…”
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Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities by Kirchschlager, Florian, Schmidt, Franziska D, Barlow, M J, Fogerty, Erica L, Bevan, Antonia, Priestley, Felix D

“…ABSTRACT The reverse shock in the ejecta of core-collapse supernovae is potentially able to destroy newly formed dust material. In order to determine dust…”
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The imprints of the last jets in core collapse supernovae by Bear, Ealeal, Grichener, Aldana, Soker, Noam

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Three Regimes and Four Modes for the Resonant Saturation of Parallel Ion-beam Instabilities by Weidl, Martin S., Winske, Dan, Niemann, Christoph

“…Motivated by recent advances in laboratory experiments on parallel ion-beam instabilities, we present a theoretical framework for-and simulations of-their…”
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The sculpting of rectangular and jet-like morphologies in supernova remnants by anisotropic equatorially confined progenitor stellar winds by Velázquez, P F, Meyer, D M-A, Chiotellis, A, Cruz-Álvarez, A E, Schneiter, E M, Toledo-Roy, J C, Reynoso, E M, Esquivel, A

“…ABSTRACT Thermonuclear and core-collapse supernova remnants (SNRs) are the nebular leftovers of defunct stars. Their morphology and emission properties provide…”
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Exploring particle escape in supernova remnants through gamma rays by Celli, S, Morlino, G, Gabici, S, Aharonian, F A

“…The escape process of particles accelerated at supernova remnant (SNR) shocks is one of the poorly understood aspects of the shock acceleration theory. Here we…”
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Three-dimensional dust mapping of 12 supernovae remnants in the Galactic anticentre by Yu, Bin, Chen, B Q, Jiang, B W, Zijlstra, A

“…ABSTRACT We present three-dimensional (3D) dust mapping of 12 supernova remnants (SNRs) in the Galactic anticentre (Galactic longitude l between 150○ and 210○)…”
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The SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM by Walch, S., Girichidis, P., Naab, T., Gatto, A., Glover, S. C. O., Wünsch, R., Klessen, R. S., Clark, P. C., Peters, T., Derigs, D., Baczynski, C.

“…The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-consistently understand the small-scale structure of the interstellar medium…”
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Progenitors and explosion properties of supernova remnants hosting central compact objects: II. A global systematic study with a comparison to nucleosynthesis models by Braun, C, Safi-Harb, S, Fryer, C L, Zhou, P

“…ABSTRACT Core-collapse explosions of massive stars leave behind neutron stars, with a known diversity that includes the ‘Central Compact Objects’ (CCOs)…”
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