Zobrazeno 1 - 10
of 4 061
pro vyhledávání: '"Mochizuki, Y"'
Autor:
Okabe, N., Umetsu, K., Tamura, T., Fujita, Y., Takizawa, M., Matsushita, K., Fukazawa, Y., Futamase, T., Kawaharada, M., Miyazaki, S., Mochizuki, Y., Nakazawa, K., Ohashi, T., Ota, N., Sasaki, T., Sato, K., Tam, S. I.
We perform a weak-lensing study of the nearby cool-core galaxy clusters, Hydra A ($z=0.0538$) and A478 ($z=0.0881$), of which brightest cluster galaxies (BCGs) host powerful activities of active galactic nuclei (AGNs). For each cluster, the observed
Externí odkaz:
http://arxiv.org/abs/1503.04412
Autor:
Homma, T. *, Mochizuki, Y., Hara, M., Kamei, S., Mizutani, T., Takubo, H., Isozaki, E., Takahashi, M., Komori, T., Hao, H.
Publikováno v:
In Revue Neurologique May 2020 176(5):353-360
Universal Profiles of the Intracluster Medium from Suzaku X-Ray and Subaru Weak Lensing Obesrvations
Autor:
Okabe, N., Umetsu, K., Tamura, T., Fujita, Y., Takizawa, M., Zhang, Y. -Y., Matsushita, K., Hamana, T., Fukazawa, Y., Futamase, T., Kawaharada, M., Miyazaki, S., Mochizuki, Y., Nakazawa, K., Ohashi, T., Ota, N., Sasaki, T., Sato, K., Tam, S. I.
We conduct a joint X-ray and weak-lensing study of four relaxed galaxy clusters (Hydra A, A478, A1689 and A1835) observed by both Suzaku and Subaru out to virial radii, with an aim to understand recently-discovered unexpected feature of the ICM in cl
Externí odkaz:
http://arxiv.org/abs/1406.3451
We review the characteristics of nucleosynthesis and radioactivities in 'Hypernovae', i.e., supernovae with very large explosion energies ($ \gsim 10^{52} $ ergs) and their $\gamma$-ray line signatures. We also discuss the $^{44}$Ti line $\gamma$-ray
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110079
Radioactive isotopes such as 44Ti offer probably the most direct probe into nucleosynthesis environments in the interior of exploding stars, when the associated gamma-ray activities in the explosion remnant are detected and translated back to the iso
Externí odkaz:
http://arxiv.org/abs/astro-ph/9904378
Publikováno v:
Astrophys.J. 492 (1998) L45
The large abundance ratio of $^{44}Ti/^{56}Ni$ in Cas A is puzzling. In fact, the ratio seems to be larger than the theoretical constraint derived by Woosley & Hoffman (1991). However, this constraint is obtained on the assumption that the explosion
Externí odkaz:
http://arxiv.org/abs/astro-ph/9807015
Publikováno v:
In CIRP Annals - Manufacturing Technology 2017 66(1):329-332
Autor:
Mochizuki, Y., Suzuki, R., Teshima, T., Matsumoto, H., Panthee, N., Sugiura, S., Hisada, T., Koyama, H.
Publikováno v:
In Journal of Veterinary Cardiology December 2016 18(4):358-366
Autor:
Suzuki, R., Mochizuki, Y., Yoshimatsu, H., Ohkusa, T., Teshima, T., Matsumoto, H., Koyama, H.
Publikováno v:
In Journal of Veterinary Cardiology December 2016 18(4):350-357
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