Zobrazeno 1 - 10
of 512
pro vyhledávání: '"Mundy, L"'
Autor:
Ginsburg, A., Csengeri, T., Galván-Madrid, R., Cunningham, N., Álvarez-Gutiérrez, R. H., Baug, T., Bonfand, M., Bontemps, S., Busquet, G., Díaz-González, D. J., Fernández-López, M., Guzmán, A., Herpin, F., Liu, H., López-Sepulcre, A., Louvet, F., Maud, L., Motte, F., Nakamura, F., Nony, T., Olguin, F. A., Pouteau, Y., Sanhueza, P., Stutz, A. M., Towner, A. P. M., Armante, M., Battersby, C., Bronfman, L., Braine, J., Brouillet, N., Chapillon, E., Di Francesco, J., Gusdorf, A., Izumi, N., Joncour, I., Lu, X., Men'shchikov, A., Menten, K. M., Moraux, E., Molet, J., Mundy, L., Luong, Q. Nguyen, Reyes-Reyes, S. D., Robitaille, J., Rosolowsky, E., Sandoval-Garrido, N. A., Svoboda, B., Tatematsu, K., Walker, D. L., Whitworth, A., Wu, B., Wyrowski, F.
Publikováno v:
A&A 662, A9 (2022)
We present the first data release of the ALMA-IMF Large Program, which covers the 12m-array continuum calibration and imaging. The ALMA-IMF Large Program is a survey of fifteen dense molecular cloud regions spanning a range of evolutionary stages tha
Externí odkaz:
http://arxiv.org/abs/2112.08183
Autor:
Motte, F., Bontemps, S., Csengeri, T., Pouteau, Y., Louvet, F., Stutz, A. M., Cunningham, N., López-Sepulcre, A., Brouillet, N., Galván-Madrid, R., Ginsburg, A., Maud, L., Men'shchikov, A., Nakamura, F., Nony, T., Sanhueza, P., Álvarez-Gutiérrez, R. H., Armante, M., Baug, T., Bonfand, M., Busquet, G., Chapillon, E., Díaz-González, D., Fernández-López, M., Guzmán, A. E., Herpin, F., Liu, H. -L., Olguin, F., Towner, A. P. M., Bally, J., Battersby, C., Braine, J., Bronfman, L., Chen, H. -R. V., Dell'Ova, P., Di Francesco, J., González, M., Gusdorf, A., Hennebelle, P., Izumi, N., Joncour, I., Lee, Y. -N., Lefloch, B., Lesaffre, P., Lu, X., Menten, K. M., Mignon-Risse, R., Molet, J., Moraux, E., Mundy, L., Luong, Q. Nguyen, Reyes, N., Reyes, S. D. Reyes, Robitaille, J. -F., Rosolowsky, E., Sandoval-Garrido, N. A., Schuller, F., Svoboda, B., Tatematsu, K., Thomasson, B., Walker, D., Wu, B., Whitworth, A. P., Wyrowski, F.
Publikováno v:
A&A 662, A8 (2022)
The ALMA-IMF Large Program imaged a total noncontiguous area of 53pc2, covering 15 extreme, nearby protoclusters of the Milky Way. They were selected to span relevant early protocluster evolutionary stages. Our 1.3mm and 3mm observations provide cont
Externí odkaz:
http://arxiv.org/abs/2112.08182
Autor:
Dipierro, G., Ricci, L., Pérez, L., Lodato, G., Alexander, R. D., Laibe, G., Andrews, S., Carpenter, J. M., Chandler, C. J., Greaves, J. A., Hall, C., Henning, T., Kwon, W., Linz, H., Mundy, L., Sargent, A., Tazzari, M., Testi, L., Wilner, D.
We present Atacama Large Millimeter/sub-millimeter Array (ALMA) Cycle 2 observations of the 1.3 mm dust continuum emission of the protoplanetary disc surrounding the T Tauri star Elias 24 with an angular resolution of $\sim 0.2"$ ($\sim 28$ au). The
Externí odkaz:
http://arxiv.org/abs/1801.05812
Autor:
Guidi, G., Tazzari, M., Testi, L., de Gregorio-Monsalvo, I., Chandler, C. J., Pérez, L., Isella, A., Natta, A., Ortolani, S., Hennings, Th., Corder, S., Linz, H., Andrews, S., Wilner, D., Ricci, L., Carpenter, J., Sargent, A., Mundy, L., Storm, S., Calvet, N., Dullemond, C., Greaves, J., Lazio, J., Deller, A., Kwon, W.
Publikováno v:
A&A 588, A112 (2016)
To characterize the mechanisms of planet formation it is crucial to investigate the properties and evolution of protoplanetary disks around young stars, where the initial conditions for the growth of planets are set. Our goal is to study grain growth
Externí odkaz:
http://arxiv.org/abs/1601.07542
Autor:
Tazzari, M., Testi, L., Ercolano, B., Natta, A., Isella, A., Chandler, C. J., Pérez, L. M., Andrews, S., Wilner, D. J., Ricci, L., Henning, T., Linz, H., Kwon, W., Corder, S. A., Dullemond, C. P., Carpenter, J. M., Sargent, A. I., Mundy, L., Storm, S., Calvet, N., Greaves, J. A., Lazio, J., Deller, A. T.
Publikováno v:
A&A 588, A53 (2016)
Theoretical models of grain growth predict dust properties to change as a function of protoplanetary disk radius, mass, age and other physical conditions. We lay down the methodology for a multi-wavelength analysis of (sub-)mm and cm continuum interf
Externí odkaz:
http://arxiv.org/abs/1512.05679
Publikováno v:
In Radiography May 2021 27(2):316-321
Autor:
Storm, S., Mundy, L. G., Fernández-López, M., Lee, K. I., Looney, L. W., Teuben, P. J., Rosolowsky, E., Arce, H. G., Ostriker, E. C., Segura-Cox, D., Pound, M. W., Salter, D. M., Volgenau, N. H., Shirley, Y. L., Chen, C., Gong, H., Plunkett, A. L., Tobin, J. J., Kwon, W., Isella, A., Kauffmann, J., Tassis, K., Crutcher, R. M., Gammie, C. F., Testi, L.
We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J=1-0 transitions) across over 800 square arcminutes of
Externí odkaz:
http://arxiv.org/abs/1409.1233
Autor:
Fernández-López, M., Arce, H. G., Looney, L., Mundy, L. G., Storm, S., Teuben, P. J., Lee, K., Segura-Cox, D., Isella, A., Tobin, J. J., Rosolowsky, E., Plunkett, A., Kwon, W., Kauffmann, J., Ostriker, E., Tassis, K., Shirley, Y. L., Pound, M.
Publikováno v:
2014, ApJ, 790, L19
We present the N2H+(J=1-0) map of the Serpens South molecular cloud obtained as part of the CARMA Large Area Star Formation Survey (CLASSy). The observations cover 250 square arcminutes and fully sample structures from 3000 AU to 3 pc with a velocity
Externí odkaz:
http://arxiv.org/abs/1407.0755
Autor:
Menu, J., van Boekel, R., Henning, T., Chandler, C. J., Linz, H., Benisty, M., Lacour, S., Min, M., Waelkens, C., Andrews, S. M., Calvet, N., Carpenter, J. M., Corder, S. A., Deller, A. T., Greaves, J. S., Harris, R. J., Isella, A., Kwon, W., Lazio, J., Bouquin, J. -B. Le, Ménard, F., Mundy, L. G., Pérez, L. M., Ricci, L., Sargent, A. I., Storm, S., Testi, L., Wilner, D. J.
For over a decade, the structure of the inner cavity in the transition disk of TW Hydrae has been a subject of debate. Modeling the disk with data obtained at different wavelengths has led to a variety of proposed disk structures. Rather than being i
Externí odkaz:
http://arxiv.org/abs/1402.6597
Autor:
Boogert, A. C. A., Chiar, J. E., Knez, C., Öberg, K. I., Mundy, L. G., Pendleton, Y. J., Tielens, A. G. G. M., van Dishoeck, E. F.
Infrared photometry and spectroscopy (1-25 um) of background stars reddened by the Lupus molecular cloud complex are used to determine the properties of the grains and the composition of the ices before they are incorporated into circumstellar envelo
Externí odkaz:
http://arxiv.org/abs/1309.2999