AHARONIAN, F., H. AKAMATSU, F. AKIMOTO, S.W. ALLEN, L. ANGELINI, M. AUDARD, H. AWAKI, M. AXELSSON, A. BAMBA, MW. BAUTZ, R. BLANDFORD, LW. BRENNEMAN, GV. BROWN, E. BULBUL, EM. CACKETT, M. CHERNYAKOVA, MP. CHIAO, PS. COPPI, E. COSTANTINI, J. DE PLAA, CP. DE VRIES, J.W. DEN HERDER, C. DONE, T. DOTANI, K. EBISAWA, ME. ECKART, T. ENOTO, Y. EZOE, A.C. FABIAN, C. FERRIGNO, A.R. FOSTER, R. FUJIMOTO, Y. FUKAZAWA, M. FURUKAWA, A. FURUZAWA, M. GALEAZZI, L.C. GALLO, P. GANDHI, M. GIUSTINI, A. GOLDWURM, Gu LY, M. GUAINAZZI, Y. HABA, K. HAGINO, K. HAMAGUCHI, IM. HARRUS, I. HATSUKADE, K. HAYASHI, T. HAYASHI, K. HAYASHIDA, JS. HIRAGA, A. HORNSCHEMEIER, A. HOSHINO, JP. HUGHES, Y. ICHINOHE, R. IIZUKA, H. INOUE, Y. INOUE, M. ISHIDA, K. ISHIKAWA, Y. ISHISAKI, M. IWAI, J. KAASTRA, T. KALLMAN, T. KAMAE, J. KATAOKA, S. KATSUDA, N. KAWAI, RL. KELLEY, CA. KILBOURNE, T. KITAGUCHI, S. KITAMOTO, T. KITAYAMA, T. KOHMURA, M. KOKUBUN, K. KOYAMA, S. KOYAMA, P. KRETSCHMAR, HA. KRIMM, A. KUBOTA, H. KUNIEDA, P. LAURENT, SH. LEE, MA. LEUTENEGGER, OO. LIMOUSIN, M. LOEWENSTEIN, KS. LONG, D. LUMB, G. MADEJSKI, Y. MAEDA, D. MAIER, K. MAKISHIMA, M. MARKEVITCH, H. MATSUMOTO, K. MATSUSHITA, D. MCCAMMON, BR. MCNAMARA, M. MEHDIPOUR, ED. MILLER, JM. MILLER, S. MINESHIGE, K. MITSUDA, I. MITSUISHI, T. MIYAZAWA, T. MIZUNO, H. MORI, K. MORI, K. MUKAI, H. MURAKAMI, R.F. MUSHOTZKY, T. NAKAGAWA, H. NAKAJIMA, T. NAKAMORI, S. NAKASHIMA, K. NAKAZAWA, KK. NORUKAWA, M. NOBUKAWA, H. NODA, H. ODAKA, A. OGORZALEK, T. OHASHI, M. OHNO, T. OKAJIMA, N. OTA, M. OZAKI, F. PAERELS, S. PALTANI, R. PETRE, C. PINTO, FS. PORTER, K. POTTSCHMIDT, C.S. REYNOLDS, S. SAFI-HARB, S. SAITO, K. SAKAI, T. SASAKI, G. SATO, K. SATO, R. SATO, M. SAWADA, N. SCHARTEL, P.J. SERLEMITSOS, H. SETA, M. SHIDATSU, A. SIMIONESCU, RK. SMITH, Y. SOONG, L. STAWARZ, Y. SUGAWARA, S. SUGITA, A. SZYMKOWIAK, H. TAJIMA, H. TAKAHASHI, T. TAKAHASHI, S. TAKEDA, Y. TAKEI, T. TAMAGAWA, T. TAMURA, T. TANAKA, Y. TANAKA, YT. TANAKA, MS. TASHIRO, Y. TAWARA, Y. TERADA, Y. TERASHIMA, F. TOMBESI, H. TOMIDA, Y. TSUBOI, M. TSUJIMOTO, H. TSUNEMI, TG. TSURU, H. UCHIDA, H. UCHIYAMA, Y. UCHIYAMA, S. UEDA, Y. UEDA, S. UNO, C.M. URRY, E. URSINO, S. WATANABE, Norbert WERNER, DR. WILKINS, BJ. WILLIAMS, S. YAMADA, H. YAMAGUCHI, K. YAMAOKA, NY. YAMASAKI, M. YAMAUCHI, S. YAMAUCHI, T. YAQOOB, Y. YATSU, D. YONETOKU, I. ZHURAVLEVA and A. ZOGHBI. Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. OXFORD: OXFORD UNIV PRESS, 2018, vol. 70, No 2, p. "10-1"-"10-29", 29 pp. ISSN 0004-6264. Available from: https://dx.doi.org/10.1093/pasj/psx127.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS
Authors AHARONIAN, F. (276 Germany), H. AKAMATSU (840 United States of America), F. AKIMOTO (840 United States of America), S.W. ALLEN (826 United Kingdom of Great Britain and Northern Ireland), L. ANGELINI (380 Italy), M. AUDARD (250 France), H. AWAKI (840 United States of America), M. AXELSSON (840 United States of America), A. BAMBA (840 United States of America), MW. BAUTZ (840 United States of America), R. BLANDFORD (826 United Kingdom of Great Britain and Northern Ireland), LW. BRENNEMAN (840 United States of America), GV. BROWN (840 United States of America), E. BULBUL (840 United States of America), EM. CACKETT (840 United States of America), M. CHERNYAKOVA (840 United States of America), MP. CHIAO (840 United States of America), PS. COPPI (840 United States of America), E. COSTANTINI (380 Italy), J. DE PLAA (528 Netherlands), CP. DE VRIES (528 Netherlands), J.W. DEN HERDER (528 Netherlands), C. DONE (826 United Kingdom of Great Britain and Northern Ireland), T. DOTANI (840 United States of America), K. EBISAWA (840 United States of America), ME. ECKART (840 United States of America), T. ENOTO (840 United States of America), Y. EZOE (840 United States of America), A.C. FABIAN (826 United Kingdom of Great Britain and Northern Ireland), C. FERRIGNO (380 Italy), A.R. FOSTER (840 United States of America), R. FUJIMOTO (840 United States of America), Y. FUKAZAWA (840 United States of America), M. FURUKAWA (840 United States of America), A. FURUZAWA (840 United States of America), M. GALEAZZI (380 Italy), L.C. GALLO (380 Italy), P. GANDHI (826 United Kingdom of Great Britain and Northern Ireland), M. GIUSTINI (380 Italy), A. GOLDWURM (840 United States of America), Gu LY (528 Netherlands), M. GUAINAZZI (380 Italy), Y. HABA (840 United States of America), K. HAGINO (840 United States of America), K. HAMAGUCHI (840 United States of America), IM. HARRUS (840 United States of America), I. HATSUKADE (840 United States of America), K. HAYASHI (840 United States of America), T. HAYASHI (840 United States of America), K. HAYASHIDA (840 United States of America), JS. HIRAGA (840 United States of America), A. HORNSCHEMEIER (840 United States of America), A. HOSHINO (840 United States of America), JP. HUGHES (840 United States of America), Y. ICHINOHE (840 United States of America), R. IIZUKA (840 United States of America), H. INOUE (840 United States of America), Y. INOUE (840 United States of America), M. ISHIDA (840 United States of America), K. ISHIKAWA (840 United States of America), Y. ISHISAKI (840 United States of America), M. IWAI (840 United States of America), J. KAASTRA (528 Netherlands), T. KALLMAN (840 United States of America), T. KAMAE (840 United States of America), J. KATAOKA (840 United States of America), S. KATSUDA (840 United States of America), N. KAWAI (840 United States of America), RL. KELLEY (840 United States of America), CA. KILBOURNE (840 United States of America), T. KITAGUCHI (840 United States of America), S. KITAMOTO (840 United States of America), T. KITAYAMA (840 United States of America), T. KOHMURA (840 United States of America), M. KOKUBUN (840 United States of America), K. KOYAMA (840 United States of America), S. KOYAMA (840 United States of America), P. KRETSCHMAR (840 United States of America), HA. KRIMM (840 United States of America), A. KUBOTA (840 United States of America), H. KUNIEDA (840 United States of America), P. LAURENT (840 United States of America), SH. LEE (250 France), MA. LEUTENEGGER (840 United States of America), OO. LIMOUSIN (250 France), M. LOEWENSTEIN (840 United States of America), KS. LONG (840 United States of America), D. LUMB (840 United States of America), G. MADEJSKI (616 Poland), Y. MAEDA (840 United States of America), D. MAIER (840 United States of America), K. MAKISHIMA (840 United States of America), M. MARKEVITCH (643 Russian Federation), H. MATSUMOTO (840 United States of America), K. MATSUSHITA (840 United States of America), D. MCCAMMON (840 United States of America), BR. MCNAMARA (840 United States of America), M. MEHDIPOUR (528 Netherlands), ED. MILLER (840 United States of America), JM. MILLER (840 United States of America), S. MINESHIGE (840 United States of America), K. MITSUDA (840 United States of America), I. MITSUISHI (840 United States of America), T. MIYAZAWA (840 United States of America), T. MIZUNO (840 United States of America), H. MORI (840 United States of America), K. MORI (840 United States of America), K. MUKAI (840 United States of America), H. MURAKAMI (840 United States of America), R.F. MUSHOTZKY (840 United States of America), T. NAKAGAWA (840 United States of America), H. NAKAJIMA (840 United States of America), T. NAKAMORI (840 United States of America), S. NAKASHIMA (840 United States of America), K. NAKAZAWA (840 United States of America), KK. NORUKAWA (840 United States of America), M. NOBUKAWA (840 United States of America), H. NODA (840 United States of America), H. ODAKA (840 United States of America), A. OGORZALEK (616 Poland), T. OHASHI (840 United States of America), M. OHNO (840 United States of America), T. OKAJIMA (840 United States of America), N. OTA (840 United States of America), M. OZAKI (840 United States of America), F. PAERELS (528 Netherlands), S. PALTANI (840 United States of America), R. PETRE (840 United States of America), C. PINTO (380 Italy), FS. PORTER (840 United States of America), K. POTTSCHMIDT (840 United States of America), C.S. REYNOLDS (826 United Kingdom of Great Britain and Northern Ireland), S. SAFI-HARB (840 United States of America), S. SAITO (840 United States of America), K. SAKAI (840 United States of America), T. SASAKI (840 United States of America), G. SATO (840 United States of America), K. SATO (840 United States of America), R. SATO (840 United States of America), M. SAWADA (840 United States of America), N. SCHARTEL (276 Germany), P.J. SERLEMITSOS (840 United States of America), H. SETA (840 United States of America), M. SHIDATSU (840 United States of America), A. SIMIONESCU (642 Romania), RK. SMITH (840 United States of America), Y. SOONG (840 United States of America), L. STAWARZ (616 Poland), Y. SUGAWARA (840 United States of America), S. SUGITA (840 United States of America), A. SZYMKOWIAK (840 United States of America), H. TAJIMA (840 United States of America), H. TAKAHASHI (840 United States of America), T. TAKAHASHI (840 United States of America), S. TAKEDA (840 United States of America), Y. TAKEI (840 United States of America), T. TAMAGAWA (840 United States of America), T. TAMURA (840 United States of America), T. TANAKA (840 United States of America), Y. TANAKA (840 United States of America), YT. TANAKA (840 United States of America), MS. TASHIRO (840 United States of America), Y. TAWARA (840 United States of America), Y. TERADA (840 United States of America), Y. TERASHIMA (840 United States of America), F. TOMBESI (380 Italy), H. TOMIDA (840 United States of America), Y. TSUBOI (840 United States of America), M. TSUJIMOTO (840 United States of America), H. TSUNEMI (840 United States of America), TG. TSURU (840 United States of America), H. UCHIDA (840 United States of America), H. UCHIYAMA (840 United States of America), Y. UCHIYAMA (840 United States of America), S. UEDA (840 United States of America), Y. UEDA (840 United States of America), S. UNO (840 United States of America), C.M. URRY (840 United States of America), E. URSINO (380 Italy), S. WATANABE (840 United States of America), Norbert WERNER (703 Slovakia, guarantor, belonging to the institution), DR. WILKINS (840 United States of America), BJ. WILLIAMS (840 United States of America), S. YAMADA (840 United States of America), H. YAMAGUCHI (840 United States of America), K. YAMAOKA (840 United States of America), NY. YAMASAKI (840 United States of America), M. YAMAUCHI (840 United States of America), S. YAMAUCHI (840 United States of America), T. YAQOOB (840 United States of America), Y. YATSU (840 United States of America), D. YONETOKU (840 United States of America), I. ZHURAVLEVA (643 Russian Federation) and A. ZOGHBI (528 Netherlands).
Edition PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, OXFORD, OXFORD UNIV PRESS, 2018, 0004-6264.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Japan
Confidentiality degree is not subject to a state or trade secret
WWW URL URL
Impact factor Impact factor: 2.750
RIV identification code RIV/00216224:14310/18:00103772
Organization unit Faculty of Science
Doi http://dx.doi.org/10.1093/pasj/psx127
UT WoS 000432287600002
Keywords in English galaxies: clusters: individual (Perseus Cluster); galaxies: clusters: intracluster medium; X-rays: galaxies: clusters
Tags International impact, Reviewed
Changed by Changed by: Mgr. Marie Šípková, DiS., učo 437722. Changed: 10/11/2022 12:50.
Abstract
Thanks to its high spectral resolution (similar to 5 eV at 6 keV), the Soft X-ray Spectrometer (SXS) on board Hitomi enables us to measure the detailed structure of spatially resolved emission lines from highly ionized ions in galaxy clusters for the first time. In this series of papers, using the SXS we have measured the velocities of gas motions, metallicities and the multi-temperature structure of the gas in the core of the Perseus Cluster. Here, we show that when inferring physical properties from line emissivities in systems like Perseus, the resonant scattering effect should be taken into account. In the Hitomi waveband, resonant scattering mostly affects the Fe XXV He alpha line (w)-the strongest line in the spectrum. The flux measured by Hitomi in this line is suppressed by a factor of similar to 1.3 in the inner similar to 30 kpc, compared to predictions for an optically thin plasma; the suppression decreases with the distance from the center. The w line also appears slightly broader than other lines from the same ion. The observed distortions of the w line flux, shape, and distance dependence are all consistent with the expected effect of the resonant scattering in the Perseus core. By measuring the ratio of fluxes in optically thick (w) and thin (Fe XXV forbidden, He beta, Ly alpha) lines, and comparing these ratios with predictions from Monte Carlo radiative transfer simulations, the velocities of gas motions have been obtained. The results are consistent with the direct measurements of gas velocities from line broadening described elsewhere in this series, although the systematic and statistical uncertainties remain significant. Further improvements in the predictions of line emissivities in plasma models, and deeper observations with future X-ray missions offering similar or better capabilities to the Hitomi SXS, will enable resonant scattering measurements to provide powerful constraints on the amplitude and anisotropy of cluster gas motions.
PrintDisplayed: 27/9/2024 08:39