Zobrazeno 1 - 10
of 2 089
pro vyhledávání: '"Low M"'
Publikováno v:
A&A 675, A38 (2023)
Context: Chondrules originate from the reprocessing of dust grains. They are key building blocks of telluric planets, yet their formation, which must happen in strongly localized regions of high temperature, remains poorly understood. Aims: We examin
Externí odkaz:
http://arxiv.org/abs/2305.16839
Autor:
Burkhart, B., Appel, S., Bialy, S., Cho, J., Christensen, A. J., Collins, D., Federrath, C., Fielding, D., Finkbeiner, D., Hill, A. S., Ibanez-Mejia, J. C., Krumholz, M. R., Lazarian, A., Li, M., Mocz, P., Mac Low, M. -M., Naiman, J., Portillo, S. K. N., Shane, B., Slepian, Z., Yuan, Y.
Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray prop
Externí odkaz:
http://arxiv.org/abs/2010.11227
Autor:
De Pree, C. G., Wilner, D. J., Kristensen, L. E., Galván-Madrid, R., Goss, W. M., Klessen, R. S., Mac Low, M. -M., Peters, T., Robinson, A., Sloman, S., Rao, M.
We present new Jansky Very Large Array (VLA) images of the central region of the W49A star-forming region at 3.6~cm and at 7~mm at resolutions of 0\farcs15 (1650 au) and 0\farcs04 (440 au), respectively. The 3.6~cm data reveal new morphological detai
Externí odkaz:
http://arxiv.org/abs/2010.04656
Autor:
Vidal, X. Cid, D'Onofrio, M., Fox, P. J., Torre, R., Ulmer, K. A., Aboubrahim, A., Albert, A., Alimena, J., Allanach, B. C., Alpigiani, C., Altakach, M., Amoroso, S., Anders, J. K., Araz, J. Y., Arbey, A., Azzi, P., Babounikau, I., Baer, H., Baker, M. J., Barducci, D., Barger, V., Baron, O., Navarro, L. Barranco, Battaglia, M., Bay, A., Bhatia, D., Biswas, S., Bloch, D., Bogavac, D., Borschensky, C., Bugge, M. K., Buttazzo, D., Cacciapaglia, G., Cadamuro, L., Calandri, A., Camargo, D. A., Canepa, A., Carminati, L., Carrá, S., Montoya, C. A. Carrillo, De Oliveira, A. Carvalho Antunes, Castillo, F. L., Cavaliere, V., Cavalli, D., Cecchi, C., Celis, A., Cerri, A., Chahal, G. S., Chakraborty, A., Chekanov, S. V., Cheng, H. J., Childers, J. T., Cirelli, M., Colegrove, O., Corcella, G., Corradi, M., Costa, M. J., Covarelli, R., Dang, N. P., Deandrea, A., De Curtis, S., De la Torre, H., Rose, L. Delle, Del Re, D., Demela, A., Demers, S., Dermisek, R., De Santo, A., Deshpande, K., Dey, B., Donini, J., Duncan, A. K., Dutta, V., Escobar, C., Fanó, L., Ferretti, G., Fiaschi, J., Fischer, O., Flacke, T., Frangipane, E. D., Frank, M., Frattari, G., Frizzell, D., Fuchs, E., Fuks, B., Gabrielli, E., Gainer, J., Gao, Y., Navarro, J. E. García, Genest, M. H., Giagu, S., Giudice, G. F., Goh, J., Gouzevitch, M., Govoni, P., Greljo, A., Grohsjean, A., Gurrola, A., Gustavino, G., Guyot, C., Gwilliam, C. B., Ha, S., Haisch, U., Haller, J., Han, T., Hayden, D., Heikinheimo, M., Heintz, U., Helsens, C., Hoepfner, K., Hogan, J. M., Huitu, K., Ilten, P., Ippolito, V., Ismail, A., Iyer, A. M., Jain, Sa., Jamin, D. O., Jeanty, L., Jezo, T., Johns, W., Kalogeropoulos, A., Karancsi, J., Kats, Y., Keller, H., Khanov, A., Kieseler, J., Kim, B., Kim, M. S., Kim, Y. G., Klasen, M., Klimek, M. D., Kogler, R., Komaragiri, J. R., Krämer, M., Kubota, S., Kulesza, A. K., Kulkarni, S., Lari, T., Ledovskoy, A., Lee, G. R., Lee, L., Lee, S. W., Leonardi, R., Les, R., Lewis, I. M., Li, Q., Li, T., Lim, I. T., Lim, S. H., Lin, K., Liu, Z., Long, K., Low, M., Lunghi, E., Madaffari, D., Mahmoudi, F., Majumder, D., Malvezzi, S., Mangano, M. L., Manoni, E., Marcano, X., Mariotti, A., Marjanovic, M., Marlow, D., Camalich, J. Martin, Cuevas, P. Matorras, McCullough, M., McDonald, E. F., Guisao, J. Mejia, Mele, B., Meloni, F., Melzer-Pellmann, I. -A., Merlassino, C., Meyer, A. B., Michielin, E., Miller, A. J., Mittnacht, L., Mondal, S., Moretti, S., Mukhopadhyay, S., Nachman, B. P., Nam, K., Narain, M., Nardecchia, M., Nath, P., Navarro-González, J., Nisati, A., Nitta, T., Noel, D. L., Nojiri, M. M., Ochoa-Ricoux, J. P., Oide, H., Ojeda, M. L., Griso, S. Pagan, Cortezon, E. Palencia, Panella, O., Pani, P., Panizzi, L., Panwar, L., Park, C. B., Pazzini, J., Pedro, K., Perego, M. M., Perrozzi, L., Petersen, B. A., Pierce, A., Polesello, G., Policicchio, A., Potter, C. J., Pralavorio, P., Presilla, M., Proudfoot, J., Queiroz, F. S., Ramirez-Sanchez, G., Redigolo, D., Reimers, A., Resconi, S., Rimoldi, M., Vergara, J. C. Rivera, Rizzo, T., Rogan, C., Romeo, F., Rosten, R., Ruiz, R., Ruiz-Alvarez, J., Iglesias, J. A. Sabater, Samani, B. Safarzadeh, Sagir, S., Saito, M., Saito, S., Sala, F., Salazar, C., Savin, A., Sawada, R., Sawant, S., Schienbein, I., Schlaffer, M., Schneider, B., Schuler, S. C., Sebastiani, C. D., Sekmen, S., Selvaggi, M., Sengupta, D., Serce, H., Serodio, H., Sestini, L., Shakya, B., Haghi, B. Shams Es, Sheldon, P., Shin, S., Simonetto, F., Soffi, L., Spannowsky, M., Stupak, J., Sullivan, M. J., Sunder, M., Takahashi, Y., Tata, X., Teagle, H., Terashi, K., Tesi, A., Thamm, A., Tobioka, K., Tornambe, P., Trovato, F., Tsiakkouri, D., Ungaro, F. C., Urbano, A., Usai, E., Vanegas, N., Vaslin, L., Sierra, C. Vázquez, Vivarelli, I., Milosavljevic, M. Vranjes, Waltari, H., Wang, R., Wang, X., Weber, M. S., Weiland, C., Wielers, M., Williams, J. M., Willocq, S., Xu, D., Yagyu, K., Yazgan, E., Ye, R., Yoo, H. D., You, T., Yu, F., Della Porta, G. Zevi, Zhang, W., Zhu, C., Zhuang, X., Zobec, J., Zupan, J., Zurita, J.
This is the third out of five chapters of the final report [1] of the Workshop on Physics at HL-LHC, and perspectives on HE-LHC [2]. It is devoted to the study of the potential, in the search for Beyond the Standard Model (BSM) physics, of the High L
Externí odkaz:
http://arxiv.org/abs/1812.07831
Autor:
De Pree, C. G., Galván-Madrid, R., Goss, W. M., Klessen, R. S., Mac Low, M. -M., Peters, T., Wilner, D., Bates, J., Melo, T., Presler-Marshall, B., Webb-Forgus, R.
A number of ultracompact H II regions in Galactic star forming environments have been observed to vary significantly in radio flux density on timescales of 10-20 years. Theory predicted that such variations should occur when the accretion flow that f
Externí odkaz:
http://arxiv.org/abs/1807.10669
Autor:
Leigh, Nathan W. C., Geller, Aaron M., McKernan, B., Ford, K. E. S., Mac Low, M. -M., Bellovary, J., Haiman, Z., Lyra, W., Samsing, J., O'Dowd, M., Kocsis, B., Endlich, S.
We assess the contribution of dynamical hardening by direct three-body scattering interactions to the rate of stellar-mass black hole binary (BHB) mergers in galactic nuclei. We derive an analytic model for the single-binary encounter rate in a nucle
Externí odkaz:
http://arxiv.org/abs/1711.10494
Publikováno v:
A&A 610, A62 (2018)
The fragmentation of filaments in molecular clouds has attracted a lot of attention as there seems to be a relation between the evolution of filaments and star formation. The study of the fragmentation process has been motivated by simple analytical
Externí odkaz:
http://arxiv.org/abs/1711.01417
Publikováno v:
In Scientific African September 2021 13
Autor:
Golling, T., Hance, M., Harris, P., Mangano, M. L., McCullough, M., Moortgat, F., Schwaller, P., Torre, R., Agrawal, P., Alves, D. S. M., Antusch, S., Arbey, A., Auerbach, B., Bambhaniya, G., Battaglia, M., Bauer, M., Dev, P. S. Bhupal, Boveia, A., Bramante, J., Buchmueller, O., Buschmann, M., Chakrabortty, J., Chala, M., Chekanov, S., Chen, C. -Y., Cheng, H. -C., Cirelli, M., Citron, M., Cohen, T., Craig, N., Curtin, D., D'Agnolo, R. T., Doglioni, C., Dror, J. A., Pree, T. du, Dylewsky, D., Ellis, J., Ellis, S. A. R., Essig, R., Fan, J. J., Farina, M., Feng, J. L., Fox, P. J., Galloway, J., Giudice, G., Gluza, J., Gori, S., Guha, S., Hahn, K., Han, T., Helsens, C., Henriques, A., Iwamoto, S., Jelinski, T., Jung, S., Kahlhoefer, F., Khoze, V. V., Kim, D., Kopp, J., Kotwal, A., Kraemer, M., Lindert, J. M., Liu, J., Lou, H. K., Love, J., Low, M., Machado, P. A. N., Mahmoudi, F., Marrouche, J., Martin, A., Mohan, K., Mohapatra, R. N., Nardini, G., Olive, K. A., Ostdiek, B., Panico, G., Plehn, T., Proudfoot, J., Qian, Z., Reece, M., Rizzo, T., Roskas, C., Ruderman, J., Ruiz, R., Sala, F., Salvioni, E., Saraswat, P., Schell, T., Schmidt-Hoberg, K., Serra, J., Shadmi, Y., Shelton, J., Solans, C., Spannowsky, M., Srivastava, T., Stolarski, D., Szafron, R., Taoso, M., Tarem, S., Thalapillil, A., Thamm, A., Tsai, Y., Verhaaren, C., Vignaroli, N., Walsh, J. R., Wang, L. T., Weiland, C., Wells, J., Williams, C., Wulzer, A., Xue, W., Yu, F., Zheng, B., Zheng, J.
This report summarises the physics opportunities in the search and study of physics beyond the Standard Model at a 100 TeV pp collider.
Comment: 196 pages, 114 figures. Chapter 3 of the "Physics at the FCC-hh" Report
Comment: 196 pages, 114 figures. Chapter 3 of the "Physics at the FCC-hh" Report
Externí odkaz:
http://arxiv.org/abs/1606.00947
Autor:
De Pree, C. G., Peters, T., Mac Low, M. -M., Wilner, D. J., Goss, W. M., Galván-Madrid, R., Keto, E. R., Klessen, R. S., Monsrud, A.
We have recently published observations of significant flux density variations at 1.3 cm in HII regions in the star forming regions Sgr B2 Main and North (De Pree et al. 2014). To further study these variations, we have made new 7 mm continuum and re
Externí odkaz:
http://arxiv.org/abs/1511.05131