Zobrazeno 1 - 10
of 122 259
pro vyhledávání: '"Walker D., A"'
Autor:
Gattis, Lyn
Publikováno v:
Technical Communication, 2023 Nov 01. 70(4), E5-E6.
Externí odkaz:
https://www.jstor.org/stable/27340678
Autor:
Nonhebel, M., Barnes, A. T., Immer, K., Armijos-Abendaño, J., Bally, J., Battersby, C., Burton, M. G., Butterfield, N., Colzi, L., García, P., Ginsburg, A., Henshaw, J. D., Hu, Y., Jiménez-Serra, I., Klessen, R. S., Kruijssen, J. M. D., Liang, F. -H., Longmore, S. N., Lu, X., Martín, S., Mills, E. A. C., Nogueras-Lara, F., Petkova, M. A., Pineda, J. E., Rivilla, V. M., Sánchez-Monge, Á., Santa-Maria, M. G., Smith, H. A., Sofue, Y., Sormani, M. C., Tolls, V., Walker, D. L., Wallace, J., Wang, Q. D., Williams, G. M., Xu, F. -W.
The Milky Way's Central Molecular Zone (CMZ) differs dramatically from our local solar neighbourhood, both in the extreme interstellar medium conditions it exhibits (e.g. high gas, stellar, and feedback density) and in the strong dynamics at play (e.
Externí odkaz:
http://arxiv.org/abs/2409.12185
Autor:
Wells, M. R. A., Beuther, H., Molinari, S., Schilke, P., Battersby, C., Ho, P., Sánchez-Monge, Á., Jones, B., Scheuck, M. B., Syed, J., Gieser, C., Kuiper, R., Elia, D., Coletta, A., Traficante, A., Wallace, J., Rigby, A. J., Klessen, R. S., Zhang, Q., Walch, S., Beltrán, M. T., Tang, Y., Fuller, G. A., Lis, D. C., Möller, T., van der Tak, F., Klaassen, P. D., Clarke, S. D., Moscadelli, L., Mininni, C., Zinnecker, H., Maruccia, Y., Pezzuto, S., Benedettini, M., Soler, J. D., Brogan, C. L., Avison, A., Sanhueza, P., Schisano, E., Liu, T., Fontani, F., Rygl, K. L. J., Wyrowski, F., Bally, J., Walker, D. L., Ahmadi, A., Koch, P., Merello, M., Law, C. Y., Testi, L.
Publikováno v:
A&A 690, A185 (2024)
We use data from the ALMA Evolutionary Study of High Mass Protocluster Formation in the Galaxy (ALMAGAL) survey to study 100 ALMAGAL regions at $\sim$ 1 arsecond resolution located between $\sim$ 2 and 6 kpc distance. Using ALMAGAL $\sim$ 1.3mm line
Externí odkaz:
http://arxiv.org/abs/2408.08299
Autor:
de Oliveira, A. G., Diamond-Hitchcock, E., Walker, D. M., Wells-Pestell, M. T., Pelegrí, G., Picken, C. J., Malcolm, G. P. A., Daley, A. J., Bass, J., Pritchard, J. D.
Neutral atom arrays have emerged as a versatile platform towards scalable quantum computation and optimization. In this paper we present demonstrations of solving maximum weighted independent set problems on a Rydberg atom array using annealing with
Externí odkaz:
http://arxiv.org/abs/2404.02658
Autor:
WEEKES, JAKE
Publikováno v:
Britannia, 2019 Jan 01. 50, 536-537.
Externí odkaz:
https://www.jstor.org/stable/26814733
Autor:
Rawat, Vineet, Samal, M. R., Eswaraiah, Chakali, Wang, Jia-Wei, Elia, Davide, Panigrahy, Sandhyarani, Zavagno, A., Yadav, R. K., Walker, D. L., Jose, J., Ojha, D. K., Zhang, C. P., Dutta, S.
The relative importance of magnetic fields, turbulence, and gravity in the early phases of star formation is still not well understood. We report the first high-resolution dust polarization observations at 850 $\mu$m around the most massive clump, lo
Externí odkaz:
http://arxiv.org/abs/2401.05310
Autor:
Rawat, Vineet, Samal, M. R., Walker, D. L., Ojha, D. K., Tej, A., Zavagno, A., Zhang, C. P., Elia, Davide, Dutta, S., Jose, J., Eswaraiah, C., Sharma, E.
Filamentary flows toward the centre of molecular clouds have been recognized as a crucial process in the formation and evolution of stellar clusters. In this paper, we present a comprehensive observational study that investigates the gas properties a
Externí odkaz:
http://arxiv.org/abs/2401.03202
Publikováno v:
Phys. Rev. Research 6, 013293 (2024)
We present an analysis of interspecies interactions between Rydberg $d$-states of rubidium and cesium. We identify the F\"orster resonance channels offering the strongest interspecies couplings, demonstrating the viability for performing high-fidelit
Externí odkaz:
http://arxiv.org/abs/2401.02308
Autor:
Walker D. Mills
Publikováno v:
The Northern Mariner / Le marin du nord. 30:67-68
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f55c25355f0a81ef6559fe4828273108
https://doi.org/10.25071/2561-5467.90
https://doi.org/10.25071/2561-5467.90
Autor:
Rawat, Vineet, Samal, M. R., Walker, D. L., Zavagno, A., Tej, A., Marton, G., Ojha, D. K., Elia, Davide, Chen, W. P., Jose, J., Eswaraiah, C
Clouds more massive than about $10^5$ M$_\odot$ are potential sites of massive cluster formation. Studying the properties of such clouds in the early stages of their evolution offers an opportunity to test various cluster formation processes. We make
Externí odkaz:
http://arxiv.org/abs/2303.05449