SIMIONESCU, Aurora, Stefano ETTORI, Norbert WERNER, Daisuke NAGAI, Franco VAZZA, Hiroki AKAMATSU, Ciro PINTO, Jelle DE PLAA, Nastasha WIJERS, Dylan NELSON, Etienne POINTECOUTEAU, Gabriel W. PRATT, Daniele SPIGA, Giuseppe VACANTI, Erwin LAU, Mariachiara ROSSETTI, Fabio GASTALDELLO, Veronica BIFFI, Esra BULBUL, Maximilien J. COLLON, Jan-Willem DEN HERDER, Dominique ECKERT, Filippo FRATERNALI, Beatriz MINGO, Giovanni PARESCHI, Gabriele PEZZULLI, Thomas H. REIPRICH, Joop SCHAYE, Stephen A. WALKER a Jessica WERK. Voyage through the hidden physics of the cosmic web. Experimental Astronomy. Springer, 2021, roč. 51, č. 3, s. 1043-1079. ISSN 0922-6435. Dostupné z: https://dx.doi.org/10.1007/s10686-021-09720-0.
Další formáty:   BibTeX LaTeX RIS
Základní údaje
Originální název Voyage through the hidden physics of the cosmic web
Autoři SIMIONESCU, Aurora (garant), Stefano ETTORI, Norbert WERNER (703 Slovensko, domácí), Daisuke NAGAI, Franco VAZZA, Hiroki AKAMATSU, Ciro PINTO, Jelle DE PLAA, Nastasha WIJERS, Dylan NELSON, Etienne POINTECOUTEAU, Gabriel W. PRATT, Daniele SPIGA, Giuseppe VACANTI, Erwin LAU, Mariachiara ROSSETTI, Fabio GASTALDELLO, Veronica BIFFI, Esra BULBUL, Maximilien J. COLLON, Jan-Willem DEN HERDER, Dominique ECKERT, Filippo FRATERNALI, Beatriz MINGO, Giovanni PARESCHI, Gabriele PEZZULLI, Thomas H. REIPRICH, Joop SCHAYE, Stephen A. WALKER a Jessica WERK.
Vydání Experimental Astronomy, Springer, 2021, 0922-6435.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Nizozemské království
Utajení není předmětem státního či obchodního tajemství
WWW URL URL
Impakt faktor Impact factor: 2.155
Kód RIV RIV/00216224:14310/21:00118981
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.1007/s10686-021-09720-0
UT WoS 000646537800001
Klíčová slova anglicky Large-scale structure; Clusters of galaxies; Circumgalactic medium; Warm-hot intergalactic medium
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 10. 11. 2022 11:39.
Anotace
The majority of the ordinary matter in the local Universe has been heated by strong structure formation shocks and resides in a largely unexplored hot, diffuse, X-ray emitting plasma that permeates the halos of galaxies, galaxy groups and clusters, and the cosmic web. We propose a next-generation “Cosmic Web Explorer” that will permit a complete and exhaustive understanding of these unseen baryons. This will be the first mission capable to reach the accretion shocks located several times farther than the virial radii of galaxy clusters, and reveal the out-of-equilibrium parts of the intra-cluster medium which are live witnesses to the physics of cosmic accretion. It will also enable a view of the thermodynamics, kinematics, and chemical composition of the circumgalactic medium in galaxies with masses similar to the Milky Way, at the same level of detail that Athena will unravel for the virialized regions of massive galaxy clusters, delivering a transformative understanding of the evolution of those galaxies in which most of the stars and metals in the Universe were formed. Finally, the proposed X-ray satellite will connect the dots of the large-scale structure by mapping, at high spectral resolution, as much as 100% of the diffuse gas hotter than 106 K that fills the filaments of the cosmic web at low redshifts, down to an over-density of 1, both in emission and in absorption against the ubiquitous cosmic X-ray background, surveying at least 1600 square degrees over 5 years in orbit. This requires a large effective area (∼ 10 m2 at 1 keV) over a large field of view (∼ 1 deg2), a megapixel cryogenic microcalorimeter array providing integral field spectroscopy with a resolving power E/ΔE = 2000 at 0.6 keV and a spatial resolution of 5′′ in the soft X-ray band, and a low and stable instrumental background ensuring high sensitivity to faint, extended emission.
Návaznosti
GX21-13491X, projekt VaVNázev: Zkoumání žhavého vesmíru a porozumění kosmické zpětné vazbě (Akronym: EHU)
Investor: Grantová agentura ČR, Exploring the Hot Universe and Understanding Comic Feedback
MUNI/I/0003/2020, interní kód MUNázev: MUNI Award in Science and Humanities 3 (Akronym: Space-Based High-Energy Astrophysics)
Investor: Masarykova univerzita, MUNI Award in Science and Humanities 3, MASH - MUNI Award in Science and Humanities
VytisknoutZobrazeno: 27. 5. 2024 10:35