Staff profile
Overview
https://apps.dur.ac.uk/biography/image/795
Research interests
- Active Galactic Nuclei (AGN), especially X-ray observation and modeling of AGN outflows
- mass loss from massive stars
Publications
Journal Article
- Geometry of the X-ray source 1H 0707–495Szanecki, M., Niedźwiecki, A., Done, C., Klepczarek, Łukasz, Lubiński, P., & Mizumoto, M. (2020). Geometry of the X-ray source 1H 0707–495. Astronomy and Astrophysics., 641, Article A89. https://doi.org/10.1051/0004-6361/202038303
- Testing the Lamp-post and Wind Reverberation Models with XMM-Newton Observations of NGC 5506Zoghbi, A., Kalli, S., Miller, J. M., & Mizumoto, M. (2020). Testing the Lamp-post and Wind Reverberation Models with XMM-Newton Observations of NGC 5506. Astrophysical Journal, 893(2), Article 97. https://doi.org/10.3847/1538-4357/ab7dc8
- Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. TaurusYasui, C., Hamano, S., Fukue, K., Kondo, S., Sameshima, H., Takenaka, K., Matsunaga, N., Ikeda, Y., Kawakita, H., Otsubo, S., Watase, A., Taniguchi, D., Mizumoto, M., Izumi, N., & Kobayashi, N. (2019). Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. Taurus. Astrophysical Journal, 886(2), Article 115. https://doi.org/10.3847/1538-4357/ab45ee
- First Detection of A–X (0,0) Bands of Interstellar C2 and CNHamano, S., Kawakita, H., Kobayashi, N., Takenaka, K., Ikeda, Y., Matsunaga, N., Kondo, S., Sameshima, H., Fukue, K., Yasui, C., Mizumoto, M., Otsubo, S., Watase, A., Yoshikawa, T., & Kobayashi, H. (2019). First Detection of A–X (0,0) Bands of Interstellar C2 and CN. Astrophysical Journal, 881(2), Article 143. https://doi.org/10.3847/1538-4357/ab2e0f
- Fe i Lines in 0.91–1.33 μm Spectra of Red Giants for Measuring the Microturbulence and MetallicitiesKondo, S., Fukue, K., Matsunaga, N., Ikeda, Y., Taniguchi, D., Kobayashi, N., Sameshima, H., Hamano, S., Arai, A., Kawakita, H., Yasui, C., Izumi, N., Mizumoto, M., Otsubo, S., Takenaka, K., Watase, A., Asano, A., Yoshikawa, T., & Tsujimoto, T. (2019). Fe i Lines in 0.91–1.33 μm Spectra of Red Giants for Measuring the Microturbulence and Metallicities. Astrophysical Journal, 875(2). https://doi.org/10.3847/1538-4357/ab0ec4
- X-ray reverberation lags of the Fe–K line due to AGN disc windsMizumoto, M., Ebisawa, K., Tsujimoto, M., Done, C., Hagino, K., & Odaka, H. (2019). X-ray reverberation lags of the Fe–K line due to AGN disc winds. Monthly Notices of the Royal Astronomical Society, 482(4), 5316-5326. https://doi.org/10.1093/mnras/sty3056
- Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter/Submillimeter Cold Molecular Outflows in Seyfert GalaxiesMizumoto, M., Izumi, T., & Kohno, K. (2019). Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter/Submillimeter Cold Molecular Outflows in Seyfert Galaxies. Astrophysical Journal, 871(2), Article 156. https://doi.org/10.3847/1538-4357/aaf814
- Thermally driven wind as the origin of warm absorbers in AGNMizumoto, M., Done, C., Tomaru, R., & Edwards, I. (2019). Thermally driven wind as the origin of warm absorbers in AGN. Monthly Notices of the Royal Astronomical Society, 489(1), 1152-1160. https://doi.org/10.1093/mnras/stz2225
- WINERED High-resolution Near-infrared Line Catalog: A-type StarSameshima, H., Ikeda, Y., Matsunaga, N., Fukue, K., Kobayashi, N., Kondo, S., Hamano, S., Kawakita, H., Yasui, C., Izumi, N., Mizumoto, M., Otsubo, S., Takenaka, K., Watase, A., Asano, A., & Yoshikawa, T. (2018). WINERED High-resolution Near-infrared Line Catalog: A-type Star. Astrophysical Journal Supplement, 239(2), Article 19. https://doi.org/10.3847/1538-4365/aae924
- A newly identified emission-line region around P CygniMizumoto, M., Kobayashi, N., Hamano, S., Ikeda, Y., Kondo, S., Sameshima, H., Matsunaga, N., Fukue, K., Yasui, C., Izumi, N., Kawakita, H., Nakanishi, K., Nakaoka, T., Otsubo, S., & Maehara, H. (2018). A newly identified emission-line region around P Cygni. Monthly Notices of the Royal Astronomical Society, 481(1), 793-805. https://doi.org/10.1093/mnras/sty2239
- X-ray short-time lags in the Fe-K energy band produced by scattering clouds in active galactic nucleiMizumoto, M., Done, C., Hagino, K., Ebisawa, K., Tsujimoto, M., & Odaka, H. (2018). X-ray short-time lags in the Fe-K energy band produced by scattering clouds in active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 478(1), 971-982. https://doi.org/10.1093/mnras/sty1114
- Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?Mizumoto, M., Moriyama, K., Ebisawa, K., Mineshige, S., Kawanaka, N., & Tsujimoto, M. (2018). Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?. Publications of Astronomical Society of Japan, 70(3), Article 42. https://doi.org/10.1093/pasj/psy032
- Nature of the warm absorber outflow in NGC 4051Mizumoto, M., & Ebisawa, K. (2017). Nature of the warm absorber outflow in NGC 4051. Monthly Notices of the Royal Astronomical Society, 466(3), 3259-3271. https://doi.org/10.1093/mnras/stw3364
- Variabiity of the X-ray broad iron spectral features in active galactic nuclei and black-hole binariesMizumoto, M., Ebisawa, K., Tsujimoto, M., & Inoue, H. (2016). Variabiity of the X-ray broad iron spectral features in active galactic nuclei and black-hole binaries. Astronomische Nachrichten, 337(4-5), 507-511. https://doi.org/10.1002/asna.201612338
- Origin of the X-ray broad iron spectral feature in GRS 1915+105Mizumoto, M., Ebisawa, K., Tsujimoto, M., & Inoue, H. (2016). Origin of the X-ray broad iron spectral feature in GRS 1915+105. Publications of Astronomical Society of Japan, 68(SP1), Article S16. https://doi.org/10.1093/pasj/psv125
- Interpretation of the X-ray spectral variation of 1H 0707−495 with a variable double partial covering modelMizumoto, M., Ebisawa, K., & Sameshima, H. (2014). Interpretation of the X-ray spectral variation of 1H 0707−495 with a variable double partial covering model. Publications of Astronomical Society of Japan, 66(6). https://doi.org/10.1093/pasj/psu121