Zobrazeno 1 - 10
of 784
pro vyhledávání: '"Tsuge K"'
Autor:
Tsuge, K., Sano, H., Tachihara, K., Bekki, K., Tokuda, K., Inoue, T., Mizuno, N., Kawamura, A., Onishi, T., Fukui, Y.
The galactic tidal interaction is a possible mechanism to trigger the active star formation in galaxies. The recent analyses using the HI data in the Large Magellanic Cloud (LMC) proposed that the tidally driven HI flow, the L-component, is colliding
Externí odkaz:
http://arxiv.org/abs/2405.05046
Autor:
Merloni, A., Lamer, G., Liu, T., Ramos-Ceja, M. E., Brunner, H., Bulbul, E., Dennerl, K., Doroshenko, V., Freyberg, M. J., Friedrich, S., Gatuzz, E., Georgakakis, A., Haberl, F., Igo, Z., Kreykenbohm, I., Liu, A., Maitra, C., Malyali, A., Mayer, M. G. F., Nandra, K., Predehl, P., Robrade, J., Salvato, M., Sanders, J. S., Stewart, I., Tubín-Arenas, D., Weber, P., Wilms, J., Arcodia, R., Artis, E., Aschersleben, J., Avakyan, A., Aydar, C., Bahar, Y. E., Balzer, F., Becker, W., Berger, K., Boller, T., Bornemann, W., Brüggen, M., Brusa, M., Buchner, J., Burwitz, V., Camilloni, F., Clerc, N., Comparat, J., Coutinho, D., Czesla, S., Dannhauer, S. M., Dauner, L., Dauser, T., Dietl, J., Dolag, K., Dwelly, T., Egg, K., Ehl, E., Freund, S., Friedrich, P., Gaida, R., Garrel, C., Ghirardini, V., Gokus, A., Grünwald, G., Grandis, S., Grotova, I., Gruen, D., Gueguen, A., Hämmerich, S., Hamaus, N., Hasinger, G., Haubner, K., Homan, D., Chitham, J. Ider, Joseph, W. M., Joyce, A., König, O., Kaltenbrunner, D. M., Khokhriakova, A., Kink, W., Kirsch, C., Kluge, M., Knies, J., Krippendorf, S., Krumpe, M., Kurpas, J., Li, P., Liu, Z., Locatelli, N., Lorenz, M., Müller, S., Magaudda, E., Mannes, C., McCall, H., Meidinger, N., Michailidis, M., Migkas, K., Muñoz-Giraldo, D., Musiimenta, B., Nguyen-Dang, N. T., Ni, Q., Olechowska, A., Ota, N., Pacaud, F., Pasini, T., Perinati, E., Pires, A. M., Pommranz, C., Ponti, G., Poppenhaeger, K., Pühlhofer, G., Rau, A., Reh, M., Reiprich, T. H., Roster, W., Saeedi, S., Santangelo, A., Sasaki, M., Schmitt, J., Schneider, P. C., Schrabback, T., Schuster, N., Schwope, A., Seppi, R., Serim, M. M., Shreeram, S., Sokolova-Lapa, E., Starck, H., Stelzer, B., Stierhof, J., Suleimanov, V., Tenzer, C., Traulsen, I., Trümper, J., Tsuge, K., Urrutia, T., Veronica, A., Waddell, S. G. H., Willer, R., Wolf, J., Yeung, M. C. H., Zainab, A., Zangrandi, F., Zhang, X., Zhang, Y., Zheng, X.
Publikováno v:
A&A, vol. 682, A34 (2024)
The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sky maps of an unprecedented depth. Here we present catalogues of both p
Externí odkaz:
http://arxiv.org/abs/2401.17274
Autor:
Sano, H., Yamane, Y., van Loon, J. Th., Furuya, K., Fukui, Y., Alsaberi, R. Z. E., Bamba, A., Enokiya, R., Filipović, M. D., Indebetouw, R., Inoue, T., Kawamura, A., Lakićević, M., Law, C. J., Mizuno, N., Murase, T., Onishi, T., Park, S., Plucinsky, P. P., Rho, J., Richards, A. M. S., Rowell, G., Sasaki, M., Seok, J., Sharda, P., Staveley-Smith, L., Suzuki, H., Temim, T., Tokuda, K., Tsuge, K., Tachihara, K.
We present the first compelling evidence of shock-heated molecular clouds associated with the supernova remnant (SNR) N49 in the Large Magellanic Cloud (LMC). Using $^{12}$CO($J$ = 2-1, 3-2) and $^{13}$CO($J$ = 2-1) line emission data taken with the
Externí odkaz:
http://arxiv.org/abs/2311.02180
Autor:
Demachi, F., Fukui, Y., Yamada, R. I., Tachihara, K., Hayakawa, T., Tokuda, K., Fujita, S., Kobayashi, M. I. N., Muraoka, K., Konishi, A., Tsuge, K., Onishi, T., Kawamura, A.
We investigated the giant molecular clouds (GMCs) in M74 (NGC 628), using data obtained from the PHANGS project. We applied the GMC Types according to the activity of star formation: Type I without star formation, Type II with H$\alpha$ luminosity ($
Externí odkaz:
http://arxiv.org/abs/2305.19192
Autor:
Yamane, Y., Sano, H., Filipovic, M. D., Tokuda, K., Fujii, K., Babazaki, Y., Mitsuishi, I., Inoue, T., Aharonian, F., Inaba, T., Inutsuka, S., Maxted, N., Mizuno, N., Onishi, T., Rowell, G., Tsuge, K., Voisin, F., Yoshiike, S., Fukuda, T., Kawamura, A., Bamba, A., Tachihara, K., Fukui, Y.
30 Doradus C is a superbubble which emits the brightest nonthermal X- and TeV gamma-rays in the Local Group. In order to explore detailed connection between the high energy radiation and the interstellar medium, we have carried out new CO and HI obse
Externí odkaz:
http://arxiv.org/abs/2106.09916
Autor:
Knies, J. R., Sasaki, M., Fukui, Y., Tsuge, K., Haberl, F., Points, S., Kavanagh, P. J., Filipović, M. D.
Publikováno v:
A&A 648, A90 (2021)
Aims: The giant HII region 30 Doradus (30 Dor) located in the eastern part of the Large Magellanic Cloud is one of the most active star-forming regions in the Local Group. Studies of HI data have revealed two large gas structures which must have coll
Externí odkaz:
http://arxiv.org/abs/2105.01437
Autor:
Sano, H., Plucinsky, P. P., Bamba, A., Sharda, P., Filipovic, M. D., Law, C. J., Alsaberi, R. Z. E., Yamane, Y., Tokuda, K., Acero, F., Sasaki, M., Vink, J., Inoue, T., Inutsuka, S., Shimoda, J., Tsuge, K., Fujii, K., Voisin, F., Maxted, N., Rowell, G., Onishi, T., Kawamura, A., Mizuno, N., Yamamoto, H., Tachihara, K., Fukui, Y.
Publikováno v:
The Astrophysical Journal, 902, 53 (2020)
N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out $^{12}$CO($J$ = 1-0, 3-2) observations toward the SNR using the Atacama Large Millimeter/submillimeter Array (ALMA) and Atacama Submillimeter
Externí odkaz:
http://arxiv.org/abs/2007.07900
LHA 115-N 83 (N83) and LHA 115-N 84 (N84) are HII regions associated with the early stage of star formation located in the Small Magellanic Cloud (SMC). We have analyzed the new HI data taken with the Galactic Australian Square Kilometre Array Pathfi
Externí odkaz:
http://arxiv.org/abs/2006.02279
NGC 602 is an outstanding young open cluster in the Small Magellanic Cloud. We have analyzed the new HI data taken with the Galactic Australian Square Kilometre Array Pathfinder survey project at an angular resolution of 30". The results show that th
Externí odkaz:
http://arxiv.org/abs/2005.13750
Autor:
Joseph, T. D., Filipović, M. D., Crawford, E. J., Bojičić, I., Alexander, E. L., Wong, G. F., Andernach, H., Leverenz, H., Norris, R. P., Alsaberi, R. Z. E., Anderson, C., Barnes, L. A., Bozzetto, L. M., Bufano, F., Bunton, J. D., Cavallaro, F., Collier, J. D., Dénes, H., Fukui, Y., Galvin, T., Haberl, F., Ingallinera, A., Kapinska, A. D., Koribalski, B. S., Kothes, R., Li, D., Maggi, P., Maitra, C., Manojlović, P., Marvil, J., Maxted, N. I., Brien, A. N. O, Oliveira, J. M., Pennock, C. M., Riggi, S., Rowell, G., Rudnick, L., Sano, H., Sasaki, M., Seymour, N., Soria, R., Stupar, M., Tothill, N. F. H., Trigilio, C., Tsuge, K., Umana, G., Urošević, D., van Loon, J. Th., Vardoulaki, E., Velović, V., Yew, M., Leahy, D., Chu, Y. -H., Micha\{l}owski, M. J., Kavanagh, P. J., Grieve, K. R.
We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small Magellanic Cloud (SMC). These images are part of the Evolutionary Map of the Universe (EMU) Early Science Pro
Externí odkaz:
http://arxiv.org/abs/1909.10425