Zobrazeno 1 - 10
of 984
pro vyhledávání: '"NOVAK G"'
Publikováno v:
Neuropsychiatric Disease and Treatment, Vol 2014, Iss default, Pp 929-952 (2014)
Mahesh N Samtani, Nandini Raghavan, Gerald Novak, Partha Nandy, Vaibhav A Narayan On behalf of the Alzheimer’s disease Neuroimaging Initiative Janssen Research and Development, LLC, Raritan, New Jersey, USA Background: The objective of this analysi
Externí odkaz:
https://doaj.org/article/af5f8eea43c14fe7b13b181a373e4b41
Autor:
Añez-López, N., Busquet, G., Koch, P. M., Girart, J. M., Liu, H. B., Santos, F., Chapman, N. L., Novak, G., Palau, A., Ho, P. T. P., Zhang, Q.
Publikováno v:
A&A 644, A52 (2020)
B-fields are predicted to play a role in the formation of filamentary structures and their fragmentation process. We aim at investigating the role of the B-field in the process of core fragmentation toward the hub-filament systems in the IRDC G14.2,
Externí odkaz:
http://arxiv.org/abs/2010.13503
Autor:
Hanany, S., Alvarez, M., Artis, E., Ashton, P., Aumont, J., Aurlien, R., Banerji, R., Barreiro, R. B., Bartlett, J. G., Basak, S., Battaglia, N., Bock, J., Boddy, K. K., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Burkhart, B., Chluba, J., Chuss, D., Clark, S., Cooperrider, J., Crill, B. P., De Zotti, G., Delabrouille, J., Di Valentino, E., Didier, J., Dore, O., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Feeney, S., Filippini, J., Fissel, L., Flauger, R., Fuskeland, U., Gluscevic, V., Gorski, K. M., Green, D., Hensley, B., Herranz, D., Hill, J. C., Hivon, E., Hlozek, R., Hubmayr, J., Johnson, B. R., Jones, W., Jones, T., Knox, L., Kogut, A., Lopez-Caniego, M., Lawrence, C., Lazarian, A., Li, Z., Madhavacheril, M., Melin, J. B., Meyers, J., Murray, C., Negrello, M., Novak, G., O'Brient, R., Paine, C., Pearson, T., Pogosian, L., Pryke, C., Puglisi, G., Remazeilles, M., Rocha, G., Schmittfull, M., Scott, D., Shirron, P., Stephens, I., Sutin, B., Tomasi, M., Trangsrud, A., van Engelen, A., Vansyngel, F., Wehus, I. K., Wen, Q., Xu, S., Young, K., Zonca, A.
The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. We describe the science achievable by PICO, which has sensitivity equiv
Externí odkaz:
http://arxiv.org/abs/1908.07495
Autor:
Lopez-Rodriguez, E., Dowell, C. D., Jones, T. J., Harper, D. A., Berthoud, M., Chuss, D., Dale, D. A., Guerra, J. A., Hamilton, R. T., Looney, L. W., Michail, J. M., Nikutta, R., Novak, G., Santos, F. P., Sheth, K., Siah, J., Staguhn, J., Stephens, I. W., Tassis, K., Trinh, C. Q., Ward-Thompson, D., Werner, M., Wollack, E. J., Zweibel, E.
We report the first detection of galactic spiral structure by means of thermal emission from magnetically aligned dust grains. Our 89 $\mu$m polarimetric imaging of NGC 1068 with the High-resolution Airborne Wideband Camera/Polarimeter (HAWC+) on NAS
Externí odkaz:
http://arxiv.org/abs/1907.06648
Akademický článek
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The relative orientation between filamentary structures in molecular clouds and the ambient magnetic field provides insight into filament formation and stability. To calculate the relative orientation, a measurement of filament orientation is first r
Externí odkaz:
http://arxiv.org/abs/1708.01953
Different combinations of input parameters to filament identification algorithms, such as Disperse and FilFinder, produce numerous different output skeletons. The skeletons are a one pixel wide representation of the filamentary structure in the origi
Externí odkaz:
http://arxiv.org/abs/1704.06377
Autor:
Soler, J. D., Ade, P. A. R., Angilè, F. E., Ashton, P., Benton, S. J., Devlin, M. J., Dober, B., Fissel, L. M., Fukui, Y., Galitzki, N., Gandilo, N. N., Hennebelle, P., Klein, J., Li, Z. -Y., Korotkov, A. L., Martin, P. G., Matthews, T. G., Moncelsi, L., Netterfield, C. B., Novak, G., Pascale, E., Poidevin, F., Santos, F. P., Savini, G., Scott, D., Shariff, J. A., Thomas, N. E., Tucker, C. E., Tucker, G. S., Ward-Thompson, D.
Publikováno v:
A&A 603, A64 (2017)
We statistically evaluate the relative orientation between gas column density structures, inferred from Herschel submillimetre observations, and the magnetic field projected on the plane of sky, inferred from polarized thermal emission of Galactic du
Externí odkaz:
http://arxiv.org/abs/1702.03853
AGN feedback from supermassive black holes (SMBHs) at the center of early type galaxies is commonly invoked as the explanation for the quenching of star formation in these systems. The situation is complicated by the significant amount of mass inject
Externí odkaz:
http://arxiv.org/abs/1511.00510
Autor:
Lo, N., Cunningham, M. R., Jones, P. A., Bronfman, L., Cortes, P. C., Simon, R., Lowe, V., Fissel, L., Novak, G.
We present first results of neutral carbon ([CI], 3P1 - 3P0 at 492 GHz) and carbon monoxide (13CO, J = 1 - 0) mapping in the Vela Molecular Ridge cloud C (VMR-C) and G333 giant molecular cloud complexes with the NANTEN2 and Mopra telescopes. For the
Externí odkaz:
http://arxiv.org/abs/1412.0476