Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS. (11th April 2018)
- Record Type:
- Journal Article
- Title:
- Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS. (11th April 2018)
- Main Title:
- Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS
- Authors:
- Aharonian, Felix
Akamatsu, Hiroki
Akimoto, Fumie
Allen, Steven W
Angelini, Lorella
Audard, Marc
Awaki, Hisamitsu
Axelsson, Magnus
Bamba, Aya
Bautz, Marshall W
Blandford, Roger
Brenneman, Laura W
Brown, Gregory V
Bulbul, Esra
Cackett, Edward M
Chernyakova, Maria
Chiao, Meng P
Coppi, Paolo S
Costantini, Elisa
de Plaa, Jelle
de Vries, Cor P
den Herder, Jan-Willem
Done, Chris
Dotani, Tadayasu
Ebisawa, Ken
Eckart, Megan E
Enoto, Teruaki
Ezoe, Yuichiro
Fabian, Andrew C
Ferrigno, Carlo
Foster, Adam R
Fujimoto, Ryuichi
Fukazawa, Yasushi
Furukawa, Maki
Furuzawa, Akihiro
Galeazzi, Massimiliano
Gallo, Luigi C
Gandhi, Poshak
Giustini, Margherita
Goldwurm, Andrea
Gu, Liyi
Guainazzi, Matteo
Haba, Yoshito
Hagino, Kouichi
Hamaguchi, Kenji
Harrus, Ilana M
Hatsukade, Isamu
Hayashi, Katsuhiro
Hayashi, Takayuki
Hayashida, Kiyoshi
Hiraga, Junko S
Hornschemeier, Ann
Hoshino, Akio
Hughes, John P
Ichinohe, Yuto
Iizuka, Ryo
Inoue, Hajime
Inoue, Yoshiyuki
Ishida, Manabu
Ishikawa, Kumi
Ishisaki, Yoshitaka
Iwai, Masachika
Kaastra, Jelle
Kallman, Tim
Kamae, Tsuneyoshi
Kataoka, Jun
Katsuda, Satoru
Kawai, Nobuyuki
Kelley, Richard L
Kilbourne, Caroline A
Kitaguchi, Takao
Kitamoto, Shunji
Kitayama, Tetsu
Kohmura, Takayoshi
Kokubun, Motohide
Koyama, Katsuji
Koyama, Shu
Kretschmar, Peter
Krimm, Hans A
Kubota, Aya
Kunieda, Hideyo
Laurent, Philippe
Lee, Shiu-Hang
Leutenegger, Maurice A
Limousin, Olivier O
Loewenstein, Michael
Long, Knox S
Lumb, David
Madejski, Greg
Maeda, Yoshitomo
Maier, Daniel
Makishima, Kazuo
Markevitch, Maxim
Matsumoto, Hironori
Matsushita, Kyoko
McCammon, Dan
McNamara, Brian R
Mehdipour, Missagh
Miller, Eric D
Miller, Jon M
Mineshige, Shin
Mitsuda, Kazuhisa
Mitsuishi, Ikuyuki
Miyazawa, Takuya
Mizuno, Tsunefumi
Mori, Hideyuki
Mori, Koji
Mukai, Koji
Murakami, Hiroshi
Mushotzky, Richard F
Nakagawa, Takao
Nakajima, Hiroshi
Nakamori, Takeshi
Nakashima, Shinya
Nakazawa, Kazuhiro
Nobukawa, Kumiko K
Nobukawa, Masayoshi
Noda, Hirofumi
Odaka, Hirokazu
Ogorzalek, Anna
Ohashi, Takaya
Ohno, Masanori
Okajima, Takashi
Ota, Naomi
Ozaki, Masanobu
Paerels, Frits
Paltani, Stéphane
Petre, Robert
Pinto, Ciro
Porter, Frederick S
Pottschmidt, Katja
Reynolds, Christopher S
Safi-Harb, Samar
Saito, Shinya
Sakai, Kazuhiro
Sasaki, Toru
Sato, Goro
Sato, Kosuke
Sato, Rie
Sawada, Makoto
Schartel, Norbert
Serlemtsos, Peter J
Seta, Hiromi
Shidatsu, Megumi
Simionescu, Aurora
Smith, Randall K
Soong, Yang
Stawarz, Łukasz
Sugawara, Yasuharu
Sugita, Satoshi
Szymkowiak, Andrew
Tajima, Hiroyasu
Takahashi, Hiromitsu
Takahashi, Tadayuki
Takeda, Shiníchiro
Takei, Yoh
Tamagawa, Toru
Tamura, Takayuki
Tanaka, Takaaki
Tanaka, Yasuo
Tanaka, Yasuyuki T
Tashiro, Makoto S
Tawara, Yuzuru
Terada, Yukikatsu
Terashima, Yuichi
Tombesi, Francesco
Tomida, Hiroshi
Tsuboi, Yohko
Tsujimoto, Masahiro
Tsunemi, Hiroshi
Tsuru, Takeshi Go
Uchida, Hiroyuki
Uchiyama, Hideki
Uchiyama, Yasunobu
Ueda, Shutaro
Ueda, Yoshihiro
Uno, Shiníchiro
Urry, C Megan
Ursino, Eugenio
Watanabe, Shin
Werner, Norbert
Wilkins, Dan R
Williams, Brian J
Yamada, Shinya
Yamaguchi, Hiroya
Yamaoka, Kazutaka
Yamasaki, Noriko Y
Yamauchi, Makoto
Yamauchi, Shigeo
Yaqoob, Tahir
Yatsu, Yoichi
Yonetoku, Daisuke
Zhuravleva, Irina
Zoghbi, Abderahmen
… (more) - Abstract:
- Abstract: Thanks to its high spectral resolution (∼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 Heα line ( w )—the strongest line in the spectrum. The flux measured by Hitomi in this line is suppressed by a factor of ∼1.3 in the inner ∼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, Heβ, Lyα) 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 gasAbstract: Thanks to its high spectral resolution (∼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 Heα line ( w )—the strongest line in the spectrum. The flux measured by Hitomi in this line is suppressed by a factor of ∼1.3 in the inner ∼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, Heβ, Lyα) 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. … (more)
- Is Part Of:
- Publications of the Astronomical Society of Japan. Volume 70(2018)Supplement 2
- Journal:
- Publications of the Astronomical Society of Japan
- Issue:
- Volume 70(2018)Supplement 2
- Issue Display:
- Volume 70, Issue 2 (2018)
- Year:
- 2018
- Volume:
- 70
- Issue:
- 2
- Issue Sort Value:
- 2018-0070-0002-0000
- Page Start:
- Page End:
- Publication Date:
- 2018-04-11
- Subjects:
- galaxies: clusters: individual (Perseus Cluster) -- galaxies: clusters: intracluster medium -- X-rays: galaxies: clusters
Astronomy -- Periodicals
520.5 - Journal URLs:
- http://pasj.asj.or.jp/ ↗
http://pasj.oxfordjournals.org/ ↗
http://www.oxfordjournals.org/ ↗ - DOI:
- 10.1093/pasj/psx127 ↗
- Languages:
- English
- ISSNs:
- 0004-6264
- Deposit Type:
- Legaldeposit
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- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 7029.000000
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