Zobrazeno 1 - 10
of 1 492
pro vyhledávání: '"Benedettini, A"'
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:
Kirk, Jason, Ward-Thompson, Derek, Di Francesco, James, André, Philippe, Bresnahan, David, Könyves, Vera, Marsh, Kenneth, Griffin, Matt, Schneider, Nicola, Men'shchikov, A., Palmeirim, Pedro, Bontemps, Sylvain, Arzoumanian, Doris, Benedettini, Milena, Pezzuto, Stefania
We present a catalogue of dense cores and filaments in a $3.8^{\circ}\times2.4^{\circ}$ field around the TMC1 region of the Taurus Molecular Cloud. The catalogue was created using photometric data from the Herschel SPIRE and PACS instruments in the 7
Externí odkaz:
http://arxiv.org/abs/2407.01233
Autor:
Hunter, Glen H., Sormani, Mattia C., Beckmann, Jan P., Vasiliev, Eugene, Glover, Simon C. O., Klessen, Ralf S., Soler, Juan D., Brucy, Noé, Girichidis, Philipp, Göller, Junia, Ohlin, Loke, Tress, Robin, Molinari, Sergio, Gerhard, Ortwin, Benedettini, Milena, Smith, Rowan, Hennebelle, Patrick, Testi, Leonardo
Obtaining reliable distance estimates to gas clouds within the Milky Way is challenging in the absence of certain tracers. The kinematic distance approach has been used as an alternative, derived from the assumption of circular trajectories around th
Externí odkaz:
http://arxiv.org/abs/2403.18000
Autor:
Colman, Tine, Brucy, Noé, Girichidis, Philipp, Glover, Simon C. O, Benedettini, Milena, Soler, Juan D., Tress, Robin G., Traficante, Alessio, Hennebelle, Patrick, Klessen, Ralf S., Molinari, Sergio, Miville-Deschênes, Marc-Antoine
Publikováno v:
A&A 686, A155 (2024)
Molecular clouds (MC) are structures of dense gas in the interstellar medium (ISM), that extend from ten to a few hundred parsecs and form the main gas reservoir available for star formation. Hydrodynamical simulations of varying complexity are a pro
Externí odkaz:
http://arxiv.org/abs/2403.00512
Autor:
Pezzuto, S., Coletta, A., Klessen, R. S., Schisano, E., Benedettini, M., Elia, D., Molinari, S., Soler, J. D., Traficante, A.
Publikováno v:
MNRAS, 525, 4744 (2023)
Many experimental quantities show a power-law distribution $p(x)\propto x^{-\alpha}$. In astrophysics, examples are: size distribution of dust grains or luminosity function of galaxies. Such distributions are characterized by the exponent $\alpha$ an
Externí odkaz:
http://arxiv.org/abs/2308.14444
Autor:
Soler, J. D., Zucker, C., Peek, J. E. G., Heyer, M., Goldsmith, P. F., Glover, S. C. O., Molinari, S., Klessen, R. S., Hennebelle, P., Testi, L., Colman, T., Benedettini, M., Elia, D., Mininni, C., Pezzuto, S., Schisano, E., Traficante, A.
Publikováno v:
A&A 675, A206 (2023)
We present a study of the three-dimensional (3D) distribution of interstellar dust derived from stellar extinction observations toward the Taurus molecular cloud (MC) and its relation with the neutral atomic hydrogen (HI) emission at 21 cm wavelength
Externí odkaz:
http://arxiv.org/abs/2305.13180
Autor:
Traficante, A., Jones, B. M., Avison, A., Fuller, G. A., Benedettini, M., Elia, D., Molinari, S., Peretto, N., Pezzuto, S., Pillai, T., Rygl, K. L. J., Schisano, E., Smith, R. J.
The formation mechanism of the most massive stars is far from completely understood. It is still unclear if the formation is core-fed or clump-fed, i.e. if the process is an extension of what happens in low-mass stars, or if the process is more dynam
Externí odkaz:
http://arxiv.org/abs/2301.09917
Autor:
Elia, D., Molinari, S., Schisano, E., Soler, J. D., Merello, M., Russeil, D., Veneziani, M., Zavagno, A., Noriega-Crespo, A., Olmi, L., Benedettini, M., Hennebelle, P., Klessen, R. S., Leurini, S., Paladini, R., Pezzuto, S., Traficante, A., Eden, D. J., Martin, P. G., Sormani, M., Coletta, A., Colman, T., Plume, R., Maruccia, Y., Mininni, C., Liu, S. J.
We present a new derivation of the Milky Way's current star formation rate (SFR) based on the data of the Hi-GAL Galactic plane survey. We estimate the distribution of the SFR across the Galactic plane from the star-forming clumps identified in the H
Externí odkaz:
http://arxiv.org/abs/2211.05573
Autor:
Riggi, S., Bordiu, C., Vitello, F., Tudisco, G., Sciacca, E., Magro, D., Sortino, R., Pino, C., Molinaro, M., Benedettini, M., Leurini, S., Bufano, F., Raciti, M., Becciani, U.
Innovative developments in data processing, archiving, analysis, and visualization are nowadays unavoidable to deal with the data deluge expected in next-generation facilities for radio astronomy, such as the Square Kilometre Array (SKA) and its prec
Externí odkaz:
http://arxiv.org/abs/2110.08211