Zobrazeno 1 - 10
of 8 766
pro vyhledávání: '"YOSHIMURA, Y."'
Autor:
Adeva, B., Afanasyev, L., Anania, A., Aogaki, S., Benelli, A., Brekhovskikh, V., Cechak, T., Chiba, M., Chliapnikov, P., Drijard, D., Dudarev, A., Dumitriu, D., Federicova, P., Gorin, A., Gritsay, K., Guaraldo, C., Gugiu, M., Hansroul, M., Hons, Z., Horikawa, S., Iwashita, Y., Kluson, J., Kobayashi, M., Kruglova, L., Kulikov, A., Kulish, E., Lamberto, A., Lanaro, A., Lednicky, R., Marinas, C., Martincik, J., Nemenov, L., Nikitin, M., Okada, K., Olchevskii, V., Pentia, M., Penzo, A., Plo, M., Prusa, P., Rappazzo, G., Vidal, A. Romero, Ryazantsev, A., Rykalin, V., Saborido, J., Schacher, J., Sidorov, A., Smolik, J., Takeutchi, F., Trojek, T., Trusov, S., Urban, T., Vrba, T., Yazkov, V., Yoshimura, Y., Zrelov, P.
In this work the Coulomb effects (Coulomb correlations) in $\pi^+\pi^-$ pairs produced in p + Ni collisions at 24 GeV/$c$, are studied using experimental $\pi^+\pi^-$ pair distributions in $Q$, the relative momentum in the pair center of mass system
Externí odkaz:
http://arxiv.org/abs/2409.12696
Autor:
Bouvier, M., Viti, S., Behrens, E., Butterworth, J., Huang, K. -Y., Mangum, J. G., Harada, N., Martín, S., Rivilla, V. M., Muller, S., Sakamoto, K., Yoshimura, Y., Tanaka, K., Nakanishi, K., Herrero-Illana, R., Colzi, L., Gorski, M. D., Henkel, C., Humire, P. K., Meier, D. S., van der Werf, P. P., Yan, Y. T.
Publikováno v:
A&A 689, A64 (2024)
Sulphur-bearing species are detected in various environments within Galactic star-forming regions and are particularly abundant in the gas phase of outflows and shocks, and photo-dissociation regions. In this work, we aim to investigate the nature of
Externí odkaz:
http://arxiv.org/abs/2405.08408
Autor:
Butterworth, J., Viti, S., Van der Werf, P. P., Mangum, J. G., Martín, S., Harada, N., Emig, K. L., Muller, S., Sakamoto, K., Yoshimura, Y., Tanaka, K., Herrero-Illana, R., Colzi, L., Rivilla, V. M., Huang, K. Y., Bouvier, M., Behrens, E., Henkel, C., Yan, Y. T., Meier, D. S., Zhou, D.
Publikováno v:
A&A 686, A31 (2024)
Determining the evolution of the CNO isotopes in the interstellar medium (ISM) of starburst galaxies can yield important constraints on the ages of superstar clusters (SSCs), or on other aspects and contributing factors of their evolution. Due to the
Externí odkaz:
http://arxiv.org/abs/2402.10721
Autor:
Huang, K. -Y., Viti, S., Holdship, J., Mangum, J. G., Martín, S., Harada, N., Muller, S., Sakamoto, K., Tanaka, K., Yoshimura, Y., Herrero-Illana, R., Meier, D. S., Behrens, E., van der Werf, P. P., Henkel, C., García-Burillo, S., Rivilla, V. M., Emig, K. L., Colzi, L., Humire, P. K., Aladro, R., Bouvier, M.
Publikováno v:
A&A 675, A151 (2023)
HNCO and SiO are well known shock tracers and have been observed in nearby galaxies, including the nearby (D=3.5 Mpc) starburst galaxy NGC 253. The simultaneous detection of these two species in regions where the star formation rate is high may be us
Externí odkaz:
http://arxiv.org/abs/2303.12685
Autor:
Humire, P. K., Henkel, C., Hernández-Gómez, A., Martín, S., Mangum, J., Harada, N., Muller, S., Sakamoto, K., Tanaka, K., Yoshimura, Y., Nakanishi, K., Mühle, S., Herrero-Illana, R., Meier, D. S., Caux, E., Aladro, R., Mauersberger, R., Viti, S., Colzi, L., Rivilla, V. M., Gorski, M., Menten, K. M., Huang, K. -Y., Aalto, S., van der Werf, P. P., Emig, K. L.
Context: Methanol masers of Class I (collisionally-pumped) and Class II (radiatively-pumped) have been studied in great detail in our Galaxy in a variety of astrophysical environments such as shocks and star-forming regions and are helpful to analyze
Externí odkaz:
http://arxiv.org/abs/2205.03281
Autor:
Adeva, B., Afanasyev, L., Anania, A., Aogaki, S., Benelli, A., Brekhovskikh, V., Cechak, T., Chiba, M., Chliapnikov, P., Drijard, D., Dudarev, A., Dumitriu, D., Federicova, P., Gorin, A., Gritsay, K., Guaraldo, C., Gugiu, M., Hansroul, M., Hons, Z., Horikawa, S., Iwashita, Y., Karpukhin, V., Kluson, J., Kobayashi, M., Kruglova, L., Kulikov, A., Kulish, E., Lamberto, A., Lanaro, A., Lednicky, R., Mariñas, C., Martincik, J., Nemenov, L., Nikitin, M., Okada, K., Olchevskii, V., Pentia, M., Penzo, A., Plo, M., Prusa, P., Rappazzo, G., Vidal, A. Romero, Ryazantsev, A., Rykalin, V., Saborido, J., Schacher, J., Sidorov, A., Smolik, J., Takeutchi, F., Trojek, T., Trusov, S., Urban, T., Vrba, T., Yazkov, V., Yoshimura, Y., Zrelov, P.
The DIRAC experiment at CERN investigated in the reaction $\rm{p}(24~\rm{GeV}/c) + Ni$ the particle pairs $K^+K^-, \pi^+ \pi^-$ and $p \bar{p}$ with relative momentum $Q$ in the pair system less than 100 MeV/c. Because of background influence studies
Externí odkaz:
http://arxiv.org/abs/2204.01857
Autor:
Machida, T., Yoshimura, Y., Nakamura, T., Kohsaka, Y., Hanaguri, T., Hsing, C. -R., Wei, C. -M., Hasegawa, Y., Hasegawa, S., Takayama, A.
Two-dimensional Rashba superconductor Si(111)-$\sqrt{3}\times\sqrt{3}$-(Tl,Pb) is a candidate platform of mixed spin-singlet and -triplet superconductivity. A recent scanning tunneling microscope (STM) experiment revealed a pseudogap at the vortex co
Externí odkaz:
http://arxiv.org/abs/2201.12721
First extragalactic detection of a phosphorus-bearing molecule with ALCHEMI: phosphorus nitride (PN)
Autor:
Haasler, D., Rivilla, V. M., Martín, S., Holdship, J., Viti, S., Harada, N., Mangum, J., Sakamoto, K., Muller, S., Tanaka, K., Yoshimura, Y., Nakanishi, K., Colzi, L., Hunt, L., Emig, K. L., Aladro, R., Humire, P., Henkel, C., van der Werf, P.
Publikováno v:
A&A 659, A158 (2022)
Phosphorus (P) is a crucial element for life given its central role in several biomolecules. P-bearing molecules have been discovered in different regions of the Milky Way, but not yet towards an extragalactic environment. We have searched for P-bear
Externí odkaz:
http://arxiv.org/abs/2112.04849
Autor:
Ito, T., Toi, K., Matsunaga, G., Isobe, M., Nagaoka, K., Takeuchi, M., Akiyama, T., Matsuoka, K., Minami, T., Nishimura, S., Okamura, S., Shimizu, A., Suzuki, C., Yoshimura, Y., Takahashi, C.
Externí odkaz:
http://hdl.handle.net/2237/14166
Autor:
Martín, S., Mangum, J. G., Harada, N., Costagliola, F., Sakamoto, K., Muller, S., Aladro, R., Tanaka, K., Yoshimura, Y., Nakanishi, K., Herrero-Illana, R., Mühle, S., Aalto, S., Behrens, E., Colzi, L., Emig, K. L., Fuller, G. A., García-Burillo, S., Greve, T. R., Henkel, C., Holdship, J., Humire, P., Hunt, L., Izumi, T., Kohno, K., König, S., Meier, D. S., Nakajima, T., Nishimura, Y., Padovani, M., Rivilla, V. M., Takano, S., van der Werf, P. P., Viti, S., Yan, Y. T.
Publikováno v:
A&A 656, A46 (2021)
We used the Atacama Large Millimeter/submillimeter Array (ALMA), covering a nearly contiguous 289 GHz frequency range between 84.2 and 373.2 GHz, to image the continuum and spectral line emission at 1.6\arcsec ($\sim 28$ pc) resolution down to a sens
Externí odkaz:
http://arxiv.org/abs/2109.08638