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pro vyhledávání: '"Moser, L"'
Autor:
Dmitriev, A.M., Razdobarin, A.G., Snigirev, L.A., Elets, D.I., Bukreev, I.M., Mukhin, E.E., Tolstyakov, S.Yu., Kupriyanov, I.B., Moser, L.
Publikováno v:
In Fusion Engineering and Design December 2024 209
Autor:
Beernaert, T.F., Verlaan, A.L., De Bock, M., Moser, L., Etman, L.F.P., Classen, I.G.J., De Baar, M.R.
Publikováno v:
In Fusion Engineering and Design August 2024 205
Autor:
Barnes, A. T., Henshaw, J. D., Fontani, F., Pineda, J. E., Cosentino, G., Tan, J. C., Caselli, P., Jiménez-Serra, I., Law, C. Y., Avison, A., Bigiel, F., Feng, S., Kong, S., Longmore, S. N., Moser, L., Parker, R. J., Sánchez-Monge, Á., Wang, K.
Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high-mass star formation (HMSF). Here we conduct an in-depth analysis of the fragmentation properties of a sample of 10 IRDCs, which have been highlighted as some of the
Externí odkaz:
http://arxiv.org/abs/2103.09122
Autor:
Liu, Daizhong, Lang, P., Magnelli, B., Schinnerer, E., Leslie, S., Fudamoto, Y., Bondi, M., Groves, B., Jimenez-Andrade, E., Harrington, K., Karim, A., Oesch, P., Sargent, M., Vardoulaki, E., Badescu, T., Moser, L., Bertoldi, F., Battisti, A., da Cunha, E., Zavala, J., Vaccari, M., Davidzon, I., Riechers, D., Aravena, M.
Publikováno v:
ApJS, 2019 October 16, Volume 244, Number 2
The rich information on (sub)millimeter dust continuum emission from distant galaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA) archive is contained in thousands of inhomogeneous observations from individual PI-led programs. T
Externí odkaz:
http://arxiv.org/abs/1910.12872
Autor:
Borkar, A., Eckart, A., Straubmeier, C., Sjouwerman, L. O., Karas, V., Kunneriath, D., Moser, L., Britzen, S., Valencia-S, M., Donea, A., Zensus, A.
We present results of 3 mm observations of SiO maser sources in the Galactic Centre (GC) from observations with the Australia Telescope Compact Array between $2010-2014$, along the transitions of the SiO molecule at $v = 1, J = 2-1$ at 86.243 GHz and
Externí odkaz:
http://arxiv.org/abs/1909.13753
Autor:
Sanchez, Fabien, Marot, L., Steiner, R., Mathys, D., Hiret, P., Soni, K., Antunes, R., Kisiel, M., Romero-Muñiz, C., Moser, L., Le Guern, F., Piqueras Meseguer, J.J., Meyer, E.
Publikováno v:
In Journal of Nuclear Materials 1 August 2023 581
Publikováno v:
Phys. Rev. B 100, 104504 (2019)
We use a scanning nanometer-scale superconducting quantum interference device (SQUID) to image individual vortices in amorphous superconducting MoSi thin films. Spatially resolved measurements of the magnetic field generated by both vortices and Meis
Externí odkaz:
http://arxiv.org/abs/1907.05110
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Autor:
Eckart, A., Valencia-S., M., Shahzamanian, B., Zajacek, M., Moser, L., Busch, G., Parsa, M., Subroweit, M., Peissker, F., Sabha, N., Hosseini, S. E., Horrobin, M., Straubmeier, C., Fazeli, N., Borkar, A., Kunneriath, D., Karas, V., Rauch, C., Britzen, S., Zensus, A., Garcia-Marin, M., Rashed, Y. E.
Bright Active Galactic Nuclei are powered by accretion of mass onto the super massive black holes at the centers of the host galaxies. For fainter objects star formation may significantly contribute to the luminosity. We summarize experimental indica
Externí odkaz:
http://arxiv.org/abs/1712.06915
Autor:
Eckart, A., Valencia-S., M., Shahzamanian, B., Zajacek, M., Moser, L., Parsa, M., Subroweit, M., Peissker, F., Sabha, N., Horrobin, M., Straubmeier, C., Borkar, A., Kunneriath, D., Karas, V., Rauch, C., Britzen, S., Zensus, A., García-Marín, M.
The Galactic Center is the closest galactic nucleus that can be studied with unprecedented angular resolution and sensitivity. We summarize recent basic observational results on Sagittarius A* and the conditions for star formation in the central stel
Externí odkaz:
http://arxiv.org/abs/1709.08963