Zobrazeno 1 - 10
of 8 205
pro vyhledávání: '"Harada, N."'
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.
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:
Gorski, M. D., Aalto, S., König, S., Wethers, C. F., Yang, C., Muller, S., Onishi, K., Sato, M., Falstad, N., Mangum, Jeffrey G., Linden, S. T., Combes, F., Martín, S., Imanishi, M., Wada, Keiichi, Barcos-Muñoz, L., Stanley, F., García-Burillo, S., van der Werf, P. P., Evans, A. S., Henkel, C., Viti, S., Harada, N., Díaz-Santos, T., Gallagher, J. S., González-Alfonso, E.
Publikováno v:
A&A 684, L11 (2024)
How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution. One potential way to regulate nuclear growth is through a galactic wind that removes gas from
Externí odkaz:
http://arxiv.org/abs/2403.16759
Autor:
Nishimura, Y., Aalto, S., Gorski, M. D., König, S., Onishi, K., Wethers, C., Yang, C., Barcos-Muñoz, L., Combes, F., Díaz-Santos, T., Gallagher, J. S., García-Burillo, S., González-Alfonso, E., Greve, T. R., Harada, N., Henkel, C., Imanishi, M., Kohno, K., Linden, S. T., Mangum, J. G., Martín, S., Muller, S., Privon, G. C., Ricci, C., Stanley, F., van der Werf, P. P., Viti, S.
Publikováno v:
A&A 686, A48 (2024)
Nuclear regions of ultraluminous and luminous infrared galaxies (U/LIRGs) are powered by starbursts and/or active galactic nuclei (AGNs). These regions are often obscured by extremely high columns of gas and dust. Molecular lines in the submillimeter
Externí odkaz:
http://arxiv.org/abs/2402.15436
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:
Abe S, Yasuda M, Tobino K, Harada S, Sasano H, Tanabe Y, Sandhu Y, Takeshige T, Matsuno K, Asao T, Sueyasu T, Nishizawa S, Yoshimine K, Ko Y, Yoshimatsu Y, Tsuruno K, Ide H, Takagi H, Ito J, Nagaoka T, Harada N, Takahashi K
Publikováno v:
Journal of Asthma and Allergy, Vol Volume 17, Pp 325-337 (2024)
Sumiko Abe,1 Mina Yasuda,1,2 Kazunori Tobino,1,2 Sonoko Harada,1,3 Hitoshi Sasano,1 Yuki Tanabe,1 Yuuki Sandhu,1 Tomohito Takeshige,1 Kei Matsuno,1 Tetsuhiko Asao,1 Takuto Sueyasu,2 Saori Nishizawa,2 Kohei Yoshimine,2 Yuki Ko,2 Yuki Yoshimatsu,2 Kosu
Externí odkaz:
https://doaj.org/article/e51c0d8c3175472d9d95738b902f3cf7
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:
Sato, M. T., Aalto, S., Kohno, K., König, S., Harada, N., Viti, S., Izumi, T., Nishimura, Y., Gorski, M.
In order to understand the evolution and feedback of Active Galactic Nuclei (AGN) and star formation it is important to use molecular lines as probes of physical conditions and chemistry. We use H$_{2}$S to investigate the impact of starburst and AGN
Externí odkaz:
http://arxiv.org/abs/2203.05851
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:
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