Zobrazeno 1 - 10
of 7 897
pro vyhledávání: '"MULLER S."'
Autor:
Wagenveld, J. D., Klöckner, H-R., Gupta, N., Sekhar, S., Jagannathan, P., Deka, P. P., Jose, J., Balashev, S. A., Borgaonkar, D., Chatterjee, A., Combes, F., Emig, K. L., Gaunekar, A. N., Hilton, M., Józsa, G. I. G., Klutse, D. Y., Knowles, K., Krogager, J. -K., Momjian, E., Muller, S., Sikhosana, S. P.
We present the second data release of the MeerKAT Absorption Line Survey (MALS), consisting of wideband continuum catalogues of 391 pointings observed at L~band. The full wideband catalogue covers 4344 deg$^2$ of sky, reaches a depth of 10 $\mu$Jy be
Externí odkaz:
http://arxiv.org/abs/2408.16619
Autor:
Grieves, N., Bouchy, F., Armstrong, D. J., Akinsanmi, B., Psaridi, A., Ulmer-Moll, S., Frensch, Y. G. C., Helled, R., Muller, S., Knierim, H., Santos, N. C., Adibekyan, V., Battley, M. P., Unger, N., Chaverot, G., Parc, L., Bayliss, D., Dumusque, X., Hawthorn, F., Figueira, P., Keniger, M. A. F., Lillo-Box, J., Nielsen, L. D., Osborn, A., Sousa, S. G., Strom, P., Udry, S.
Hot Jupiters generally do not have nearby planet companions, as they may have cleared out other planets during their inward migration from more distant orbits. This gives evidence that hot Jupiters more often migrate inward via high-eccentricity migr
Externí odkaz:
http://arxiv.org/abs/2406.15986
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:
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:
Wethers, C. F., Aalto, S., Privon, G. C., Stanley, F., Gallagher, J., Gorski, M., König, S., Onishi, K., Sato, M., Yang, C., Beswick, R., Combes, L. Barcos-Munoz F., Diaz-Santos, T., Evans, A. S., Garcia-Bernete, I., Henkel, C., Imanishi, M., Martín, S., Muller, S., Nishimura, Y., Ricci, C., Rigopoulou, D., Viti, S.
Compact obscured nuclei (CONs) are an extremely obscured (N$_{H2}$ >10$^{25}$ cm$^{-2}$) class of galaxy nuclei thought to exist in 20-40 per cent of nearby (ultra-)luminous infrared galaxies. While they have been proposed to represent a key phase of
Externí odkaz:
http://arxiv.org/abs/2402.17590
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:
Corrodi, S., Oksuzian, Y., Edmonds, A., Miller, J., Tran, H. N., Bonventre, R., Brown, D. N., Meot, F., Singh, V., Kolomensky, Y., Tripathy, S., Borrel, L., Bub, M., Echenard, B., Hitlin, D. G., Jafree, H., Middleton, S., Plestid, R., Porter, F. C., Zhu, R. Y., Bottura, L., Pinsard, E., Teixeira, A. M., Carelli, C., Ambrose, D., Badgley, K., Bautista, G. D., Bernstein, R. H., Boi, S., Crnkovic, J., Eldred, J., Gaponenko, A., Johnstone, C., Kiburg, B., Kutschke, R., Lynch, K., Mukherjee, A., Neuffer, D., Pellemoine, F., Pronskikh, V., Rakness, G., Tang, J., Tschirhart, R., Yucel, M., Zettlemoyer, J., Simons, B., Redigolo, D., Diociaiuti, E., Giovannella, S., Miscetti, S., Sarra, I., Muller, S. E., Ootani, W., Yucel, E. B., Kaplan, D. M., Phillips, T. J., Pasternak, J., Palo, D., Davydov, Y., Brown, D., Banerjee, S., Kawall, D., Hartwig, Z., Davidson, S., Abrams, R., Kampa, C., Mackenzie, M., Schmitt, M., Piot, P., Lee, Y. J., Morozov, V., Sato, A., Di Falco, S., Gioiosa, A., Morescalchi, L., Papa, A., Hedges, M. T., Renga, F., Lagrange, J. -B., Rogers, C., Wilcox, D., Petrov, A., Zhao, S., Dukes, E. C., Erlich, R., Group, C., Heeck, J., Pezzullo, G., Nguyen, T., Popp, J. L.
The Snowmass report on rare processes and precision measurements recommended Mu2e-II and a next generation muon facility at Fermilab (Advanced Muon Facility) as priorities for the frontier. The Workshop on a future muon program at FNAL was held in Ma
Externí odkaz:
http://arxiv.org/abs/2309.05933
Autor:
Muller, S., Marti-Vidal, I., Combes, F., Gerin, M., Beelen, A., Horellou, C., Guelin, M., Aalto, S., Black, J. H., van Kampen, E.
Publikováno v:
A&A 674, A101 (2023)
Time variability of astronomical sources provides crude information on their typical size and on the implied physical mechanisms. PKS1830-211 is a remarkable radio-bright lensed quasar with a foreground molecular absorber at z=0.89. Small-scale morph
Externí odkaz:
http://arxiv.org/abs/2304.09002