Zobrazeno 1 - 10
of 815
pro vyhledávání: '"MERELLO, M."'
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
Publikováno v:
A&A 677, A148 (2023)
(Abridged) High-mass star formation is far less understood than low-mass star formation. It entails molecular outflows, which disturb the protostellar clump. Studying these outflows and the shocked gas they cause is key for a better understanding of
Externí odkaz:
http://arxiv.org/abs/2307.16350
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:
Benedettini, M., Traficante, A., Olmi, L., Pezzuto, S., Baldeschi, A., Molinari, S., Elia, D., Schisano, E., Merello, M., Fontani, F., Rygl, K. L. J., Brand, J., Beltran, M. T., Cesaroni, R., Liu, S. J., Testi, L.
Publikováno v:
A&A 654, A144 (2021)
New-generation spectroscopic surveys of the Milky Way plane have been revealing the structure of the interstellar medium, allowing the simultaneous study of dense structures from single star-forming objects or systems to entire spiral arms. We presen
Externí odkaz:
http://arxiv.org/abs/2109.00950
Autor:
Elia, D., Merello, M., Molinari, S., Schisano, E., Zavagno, A., Russeil, D., Mège, P., Martin, P. G., Olmi, L., Pestalozzi, M., Plume, R., Ragan, S. E., Benedettini, M., Eden, D. J., Moore, T. J. T., Noriega-Crespo, A., Paladini, R., Palmeirim, P., Pezzuto, S., Pilbratt, G. L., Rygl, K. L. J., Schilke, P., Strafella, F., Tan, J. C., Traficante, A., Baldeschi, A., Bally, J., di Giorgio, A. M., Fiorellino, E., Liu, S. J., Piazzo, L., Polychroni, D.
We present the $360^\circ$ catalogue of physical properties of Hi-GAL compact sources, detected between 70 and 500 $\mu$m. This release not only completes the analogous catalogue previously produced by the Hi-GAL collaboration for $-71^\circ \lesssim
Externí odkaz:
http://arxiv.org/abs/2104.04807
Autor:
Jones, B. M., Fuller, G. A., Breen, S. L., Avison, A., Green, J. A., Traficante, A., Elia, D., Ellingsen, S. P., Voronkov, M. A., Merello, M., Molinari, S., Schisano, E.
The Methanol MultiBeam survey (MMB) provides the most complete sample of Galactic massive young stellar objects (MYSOs) hosting 6.7GHz class II methanol masers. We characterise the properties of these maser sources using dust emission detected by the
Externí odkaz:
http://arxiv.org/abs/2001.08449
Autor:
Schisano, E., Molinari, S., Elia, D., Benedettini, M., Olmi, L., Pezzuto, S., Traficante, A., Brescia, M., Cavuoti, S., di Giorgio, A. M., Liu, S. J., Moore, T. J. T., Noriega-Crespo, A., Riccio, G., Baldeschi, A., Becciani, U., Peretto, N., Merello, M., Vitello, F., Zavagno, A., Beltrán, M. T., Cambrésy, L., Eden, D. J., Causi, G. Li, Molinaro, M., Palmeirim, P., Sciacca, E., Testi, L., Umana, G., Whitworth, A. P.
The recent data collected by {\it Herschel} have confirmed that interstellar structures with filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to be formed by several physical mechanisms acting from the large Galactic
Externí odkaz:
http://arxiv.org/abs/1912.04020
Autor:
Benedettini, M., Molinari, S., Baldeschi, A., Beltran, M. T., Brand, J., Cesaroni, R., Elia, D., Fontani, F., Merello, M., Olmi, L., Pezzuto, S., Rygl, K. L. J., Schisano, E., Testi, L., Traficante, A.
Publikováno v:
A&A 633, A147 (2020)
We present the Forgotten Quadrant Survey (FQS), an ESO large project that used the 12m antenna of the Arizona Radio Observatory to map the Galactic Plane in the range 220\deg$
Externí odkaz:
http://arxiv.org/abs/1911.11545
Autor:
Duronea, N. U., Bronfman, L., Mendoza, E., Merello, M., Finger, R., Reyes, N., Hervías-Caimapo, C., Faure, A., Cappa, C. E., Arnal, E. M., Lépine, J. R. D., Kleiner, I., Nyman, L-Ä
Using APEX-1 and APEX-2 observations, we have detected and studied the rotational lines of the HC$_3$N molecule (cyanoacetylene) in the powerful outflow/hot molecular core G331.512-0.103. We identified thirty-one rotational lines at $J$ levels betwee
Externí odkaz:
http://arxiv.org/abs/1907.09479
Autor:
Molinari, S., Baldeschi, A., Robitaille, T. P., Morales, E. F. E., Schisano, E., Traficante, A., Merello, M., Molinaro, M., Vitello, F., Sciacca, E., Liu, S. J.
A grid of 20 millions 3-1100$\mu$m SED models is presented for synthetic young clusters embedded in dense clumps. The models depend on four primary parameters: the clump mass M$_{clump}$ and dust temperature T$_{dust}$, the fraction of mass f$_{core}
Externí odkaz:
http://arxiv.org/abs/1904.08140