Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta
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AHARONIAN, F.; H. AKAMATSU; F. AKIMOTO; SW 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; JW DEN HERDER; C. DONE; T. DOTANI; K. EBISAWA; ME ECKART; T. ENOTO; Y. EZOE; AC FABIAN; C. FERRIGNO; AR FOSTER; R. FUJIMOTO; Y. FUKAZAWA; A. FURUZAWA; M. GALEAZZI; LC 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; O. 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; RF MUSHOTZKY; T. NAKAGAWA; H. NAKAJIMA; T. NAKAMORI; S. NAKASHIMA; K. NAKAZAWA; KK NORUKAWA; M. NOBUKAWA; H. NODA; H. ODAKA; T. OHASHI; M. OHNO; T. OKAJIMA; N. OTA; M. OZAKI; F. PAERELS; S. PALTANI; R. PETRE; C. PINTO; FS PORTER; K. POTTSCHMIDT; CS REYNOLDS; S. SAFI-HARB; S. SAITO; K. SAKAI; T. SASAKI; G. SATO; K. SATO; R. SATO; T. SATO; M. SAWADA; N. SCHARTEL; PJ 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; CM 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 a A. ZOGHBI
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PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, OXFORD, OXFORD UNIV PRESS, 2018, 0004-6264
We present Hitomi observations of N 132 D, a young, X-ray bright, O-rich core-collapse supernova remnant in the Large Magellanic Cloud (LMC). Despite a very short observation of only 3.7 ks, the Soft X-ray Spectrometer (SXS) easily detects the line complexes of highly ionized S K and Fe K with 16-17 counts in each. The Fe feature is measured for the first time at high spectral resolution. Based on the plausible assumption that the Fe K emission is dominated by He-like ions, we find that the material responsible for this Fe emission is highly redshifted at similar to 800 km s(-1) compared to the local LMC interstellar medium (ISM), with a 90% credible interval of 50-1500 km s(-1) if a weakly informative prior is placed on possible line broadening. This indicates (1) that the Fe emission arises from the supernova ejecta, and (2) that these ejecta are highly asymmetric, since no blueshifted component is found. The S K velocity is consistent with the local LMC ISM, and is likely from swept-up ISM material. These results are consistent with spatial mapping that shows the He-like Fe concentrated in the interior of the remnant and the S tracing the outer shell. The results also show that even with a very small number of counts, direct velocity measurements from Doppler-shifted lines detected in extended objects like supernova remnants are now possible. Thanks to the very low SXS background of similar to 1 event per spectral resolution element per 100 ks, such results are obtainable during short pointed or slew observations with similar instruments. This highlights the power of high-spectral-resolution imaging observations, and demonstrates the new window that has been opened with Hitomi and will be greatly widened with future missions such as the X-ray Astronomy Recovery Mission (XARM) and Athena.
AHARONIAN, F.; H. AKAMATSU; F. AKIMOTO; SW 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; JW DEN HERDER; C. DONE; T. DOTANI; K. EBISAWA; ME ECKART; T. ENOTO; Y. EZOE; AC FABIAN; C. FERRIGNO; AR FOSTER; R. FUJIMOTO; Y. FUKAZAWA; A. FURUZAWA; M. GALEAZZI; LC 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; O. 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; RF MUSHOTZKY; T. NAKAGAWA; H. NAKAJIMA; T. NAKAMORI; S. NAKASHIMA; K. NAKAZAWA; KK NORUKAWA; M. NOBUKAWA; H. NODA; H. ODAKA; T. OHASHI; M. OHNO; T. OKAJIMA; N. OTA; M. OZAKI; F. PAERELS; S. PALTANI; R. PETRE; C. PINTO; FS PORTER; K. POTTSCHMIDT; CS REYNOLDS; S. SAFI-HARB; S. SAITO; K. SAKAI; T. SASAKI; G. SATO; K. SATO; R. SATO; T. SATO; M. SAWADA; N. SCHARTEL; PJ 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; CM 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 a A. ZOGHBI. Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. OXFORD: OXFORD UNIV PRESS, 2018, roč. 70, č. 2, s. "16-1"-"16-19", 19 s. ISSN 0004-6264. Dostupné z: https://doi.org/10.1093/pasj/psx151.
@article{1444559, author = {Aharonian, F. and Akamatsu, H. and Akimoto, F. and Allen, SW and Angelini, L. and Audard, M. and Awaki, H. and Axelsson, M. and Bamba, A. and Bautz, MW and Blandford, R. and Brenneman, LW and Brown, GV and Bulbul, E. and Cackett, EM and Chernyakova, M. and Chiao, MP and Coppi, PS and Costantini, E. and de Plaa, J. and de Vries, CP and den Herder, JW and Done, C. and Dotani, T. and Ebisawa, K. and Eckart, ME and Enoto, T. and Ezoe, Y. and Fabian, AC and Ferrigno, C. and Foster, AR and Fujimoto, R. and Fukazawa, Y. and Furuzawa, A. and Galeazzi, M. and Gallo, LC and Gandhi, P. and Giustini, M. and Goldwurm, A. and LY, Gu and Guainazzi, M. and Haba, Y. and Hagino, K. and Hamaguchi, K. and Harrus, IM and Hatsukade, I. and Hayashi, K. and Hayashi, T. and Hayashida, K. and Hiraga, JS and Hornschemeier, A. and Hoshino, A. and Hughes, JP and Ichinohe, Y. and Iizuka, R. and Inoue, H. and Inoue, Y. and Ishida, M. and Ishikawa, K. and Ishisaki, Y. and Iwai, M. and Kaastra, J. and Kallman, T. and Kamae, T. and Kataoka, J. and Katsuda, S. and Kawai, N. and Kelley, RL and Kilbourne, CA and Kitaguchi, T. and Kitamoto, S. and Kitayama, T. and Kohmura, T. and Kokubun, M. and Koyama, K. and Koyama, S. and Kretschmar, P. and Krimm, HA and Kubota, A. and Kunieda, H. and Laurent, P. and Lee, SH and Leutenegger, MA and Limousin, O. and Loewenstein, M. and Long, KS and Lumb, D. and Madejski, G. and Maeda, Y. and Maier, D. and Makishima, K. and Markevitch, M. and Matsumoto, H. and Matsushita, K. and McCammon, D. and McNamara, BR and Mehdipour, M. and Miller, ED and Miller, JM and Mineshige, S. and Mitsuda, K. and Mitsuishi, I. and Miyazawa, T. and Mizuno, T. and Mori, H. and Mori, K. and Mukai, K. and Murakami, H. and Mushotzky, RF and Nakagawa, T. and Nakajima, H. and Nakamori, T. and Nakashima, S. and Nakazawa, K. and Norukawa, KK and Nobukawa, M. and Noda, H. and Odaka, H. and Ohashi, T. and Ohno, M. and Okajima, T. and Ota, N. and Ozaki, M. and Paerels, F. and Paltani, S. and Petre, R. and Pinto, C. and Porter, FS and Pottschmidt, K. and Reynolds, CS and SafiandHarb, S. and Saito, S. and Sakai, K. and Sasaki, T. and Sato, G. and Sato, K. and Sato, R. and Sato, T. and Sawada, M. and Schartel, N. and Serlemitsos, PJ and Seta, H. and Shidatsu, M. and Simionescu, A. and Smith, RK and Soong, Y. and Stawarz, L. and Sugawara, Y. and Sugita, S. and Szymkowiak, A. and Tajima, H. and Takahashi, H. and Takahashi, T. and Takeda, S. and Takei, Y. and Tamagawa, T. and Tamura, T. and Tanaka, T. and Tanaka, Y. and Tanaka, YT and Tashiro, MS and Tawara, Y. and Terada, Y. and Terashima, Y. and Tombesi, F. and Tomida, H. and Tsuboi, Y. and Tsujimoto, M. and Tsunemi, H. and Tsuru, TG and Uchida, H. and Uchiyama, H. and Uchiyama, Y. and Ueda, S. and Ueda, Y. and Uno, S. and Urry, CM and Ursino, E. and Watanabe, S. and Werner, Norbert and Wilkins, DR and Williams, BJ and Yamada, S. and Yamaguchi, H. and Yamaoka, K. and Yamasaki, NY and Yamauchi, M. and Yamauchi, S. and Yaqoob, T. and Yatsu, Y. and Yonetoku, D. and Zhuravleva, I. and Zoghbi, A.}, article_location = {OXFORD}, article_number = {2}, doi = {https://doi.org/10.1093/pasj/psx151}, keywords = {ISM: individual objects (N 132 D); ISM: supernova remnants; instrumentation: spectrographs; methods: observational; X-rays: individual (N 132 D)}, language = {eng}, issn = {0004-6264}, journal = {PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN}, title = {Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta}, url = {https://academic.oup.com/pasj/article/70/2/16/4969727}, volume = {70}, year = {2018} }
TY - JOUR ID - 1444559 AU - Aharonian, F. - Akamatsu, H. - Akimoto, F. - Allen, SW - Angelini, L. - Audard, M. - Awaki, H. - Axelsson, M. - Bamba, A. - Bautz, MW - Blandford, R. - Brenneman, LW - Brown, GV - Bulbul, E. - Cackett, EM - Chernyakova, M. - Chiao, MP - Coppi, PS - Costantini, E. - de Plaa, J. - de Vries, CP - den Herder, JW - Done, C. - Dotani, T. - Ebisawa, K. - Eckart, ME - Enoto, T. - Ezoe, Y. - Fabian, AC - Ferrigno, C. - Foster, AR - Fujimoto, R. - Fukazawa, Y. - Furuzawa, A. - Galeazzi, M. - Gallo, LC - Gandhi, P. - Giustini, M. - Goldwurm, A. - LY, Gu - Guainazzi, M. - Haba, Y. - Hagino, K. - Hamaguchi, K. - Harrus, IM - Hatsukade, I. - Hayashi, K. - Hayashi, T. - Hayashida, K. - Hiraga, JS - Hornschemeier, A. - Hoshino, A. - Hughes, JP - Ichinohe, Y. - Iizuka, R. - Inoue, H. - Inoue, Y. - Ishida, M. - Ishikawa, K. - Ishisaki, Y. - Iwai, M. - Kaastra, J. - Kallman, T. - Kamae, T. - Kataoka, J. - Katsuda, S. - Kawai, N. - Kelley, RL - Kilbourne, CA - Kitaguchi, T. - Kitamoto, S. - Kitayama, T. - Kohmura, T. - Kokubun, M. - Koyama, K. - Koyama, S. - Kretschmar, P. - Krimm, HA - Kubota, A. - Kunieda, H. - Laurent, P. - Lee, SH - Leutenegger, MA - Limousin, O. - Loewenstein, M. - Long, KS - Lumb, D. - Madejski, G. - Maeda, Y. - Maier, D. - Makishima, K. - Markevitch, M. - Matsumoto, H. - Matsushita, K. - McCammon, D. - McNamara, BR - Mehdipour, M. - Miller, ED - Miller, JM - Mineshige, S. - Mitsuda, K. - Mitsuishi, I. - Miyazawa, T. - Mizuno, T. - Mori, H. - Mori, K. - Mukai, K. - Murakami, H. - Mushotzky, RF - Nakagawa, T. - Nakajima, H. - Nakamori, T. - Nakashima, S. - Nakazawa, K. - Norukawa, KK - Nobukawa, M. - Noda, H. - Odaka, H. - Ohashi, T. - Ohno, M. - Okajima, T. - Ota, N. - Ozaki, M. - Paerels, F. - Paltani, S. - Petre, R. - Pinto, C. - Porter, FS - Pottschmidt, K. - Reynolds, CS - Safi-Harb, S. - Saito, S. - Sakai, K. - Sasaki, T. - Sato, G. - Sato, K. - Sato, R. - Sato, T. - Sawada, M. - Schartel, N. - Serlemitsos, PJ - Seta, H. - Shidatsu, M. - Simionescu, A. - Smith, RK - Soong, Y. - Stawarz, L. - Sugawara, Y. - Sugita, S. - Szymkowiak, A. - Tajima, H. - Takahashi, H. - Takahashi, T. - Takeda, S. - Takei, Y. - Tamagawa, T. - Tamura, T. - Tanaka, T. - Tanaka, Y. - Tanaka, YT - Tashiro, MS - Tawara, Y. - Terada, Y. - Terashima, Y. - Tombesi, F. - Tomida, H. - Tsuboi, Y. - Tsujimoto, M. - Tsunemi, H. - Tsuru, TG - Uchida, H. - Uchiyama, H. - Uchiyama, Y. - Ueda, S. - Ueda, Y. - Uno, S. - Urry, CM - Ursino, E. - Watanabe, S. - Werner, Norbert - Wilkins, DR - Williams, BJ - Yamada, S. - Yamaguchi, H. - Yamaoka, K. - Yamasaki, NY - Yamauchi, M. - Yamauchi, S. - Yaqoob, T. - Yatsu, Y. - Yonetoku, D. - Zhuravleva, I. - Zoghbi, A. PY - 2018 TI - Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta JF - PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN VL - 70 IS - 2 SP - "16-1"-"16-19" EP - "16-1"-"16-19" PB - OXFORD UNIV PRESS SN - 00046264 KW - ISM: individual objects (N 132 D) KW - ISM: supernova remnants KW - instrumentation: spectrographs KW - methods: observational KW - X-rays: individual (N 132 D) UR - https://academic.oup.com/pasj/article/70/2/16/4969727 N2 - We present Hitomi observations of N 132 D, a young, X-ray bright, O-rich core-collapse supernova remnant in the Large Magellanic Cloud (LMC). Despite a very short observation of only 3.7 ks, the Soft X-ray Spectrometer (SXS) easily detects the line complexes of highly ionized S K and Fe K with 16-17 counts in each. The Fe feature is measured for the first time at high spectral resolution. Based on the plausible assumption that the Fe K emission is dominated by He-like ions, we find that the material responsible for this Fe emission is highly redshifted at similar to 800 km s(-1) compared to the local LMC interstellar medium (ISM), with a 90% credible interval of 50-1500 km s(-1) if a weakly informative prior is placed on possible line broadening. This indicates (1) that the Fe emission arises from the supernova ejecta, and (2) that these ejecta are highly asymmetric, since no blueshifted component is found. The S K velocity is consistent with the local LMC ISM, and is likely from swept-up ISM material. These results are consistent with spatial mapping that shows the He-like Fe concentrated in the interior of the remnant and the S tracing the outer shell. The results also show that even with a very small number of counts, direct velocity measurements from Doppler-shifted lines detected in extended objects like supernova remnants are now possible. Thanks to the very low SXS background of similar to 1 event per spectral resolution element per 100 ks, such results are obtainable during short pointed or slew observations with similar instruments. This highlights the power of high-spectral-resolution imaging observations, and demonstrates the new window that has been opened with Hitomi and will be greatly widened with future missions such as the X-ray Astronomy Recovery Mission (XARM) and Athena. ER -
AHARONIAN, F.; H. AKAMATSU; F. AKIMOTO; SW 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; JW DEN HERDER; C. DONE; T. DOTANI; K. EBISAWA; ME ECKART; T. ENOTO; Y. EZOE; AC FABIAN; C. FERRIGNO; AR FOSTER; R. FUJIMOTO; Y. FUKAZAWA; A. FURUZAWA; M. GALEAZZI; LC 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; O. 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; RF MUSHOTZKY; T. NAKAGAWA; H. NAKAJIMA; T. NAKAMORI; S. NAKASHIMA; K. NAKAZAWA; KK NORUKAWA; M. NOBUKAWA; H. NODA; H. ODAKA; T. OHASHI; M. OHNO; T. OKAJIMA; N. OTA; M. OZAKI; F. PAERELS; S. PALTANI; R. PETRE; C. PINTO; FS PORTER; K. POTTSCHMIDT; CS REYNOLDS; S. SAFI-HARB; S. SAITO; K. SAKAI; T. SASAKI; G. SATO; K. SATO; R. SATO; T. SATO; M. SAWADA; N. SCHARTEL; PJ 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; CM 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 a A. ZOGHBI. Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta. \textit{PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN}. OXFORD: OXFORD UNIV PRESS, 2018, roč.~70, č.~2, s.~''16-1''-''16-19'', 19 s. ISSN~0004-6264. Dostupné z: https://doi.org/10.1093/pasj/psx151.