Zobrazeno 1 - 10
of 517
pro vyhledávání: '"OLMI L"'
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:
Roshi, D. Anish, Aponte, N., Araya, E., Arce, H., Baker, L. A., Baan, W., Becker, T. M., Breakall, J. K., Brown, R. G., Brum, C. G. M., Busch, M., Campbell, D. B., Cohen, T., Cordova, F., Deneva, J. S., Devogele, M., Dolch, T., Fernandez-Rodriguez, F. O., Ghosh, T., Goldsmith, P. F., Gurvits, L. I., Haynes, M., Heiles, C., Hessel, J. W. T., Hickson, D., Isham, B., Kerr, R. B., Kelly, J., Kiriazes, J. J., Lautenbach, J., Lebron, M., Lewandowska, N., Magnani, L., Manoharan, P. K., Margot, J. L., Marshall, S. E., McGilvray, A. K., Mendez, A., Minchin, R., Negron, V., Nolan, M. C., Olmi, L., Paganelli, F., Palliyaguru, N. T., Pantoja, C. A., Paragi, Z., Parshley, S. C., Peek, J. E. G., Perera, B. B. P., Perillat, P., Pinilla-Alonso, N., Quintero, L., Radovan, H., Raizada, S., Robishaw, T., Route, M., Salter, C. J., Santoni, A., Santos, P., Sau, S., Selvaraj, D., Smith, A. J., Sulzer, M., Vaddi, S., Vargas, F., Venditti, F. C. F., Venkataraman, A., Verkouter, H., Virkki, A. K., Vishwas, A., Weinreb, S., Werthimer, D., Wolszczan, A., Zambrano-Marin, L. F.
The Arecibo Observatory (AO) is a multidisciplinary research and education facility that is recognized worldwide as a leading facility in astronomy, planetary, and atmospheric and space sciences. AO's cornerstone research instrument was the 305-m Wil
Externí odkaz:
http://arxiv.org/abs/2103.01367
We report on one of the highest sensitivity surveys for molecular lines in the frequency range 6.0 to 7.4 GHz conducted to date. The observations were done with the 305m Arecibo Telescope toward a sample of twelve intermediate/high-mass star forming
Externí odkaz:
http://arxiv.org/abs/2006.11817
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:
Massi, F., Weiss, A., Elia, D., Csengeri, T., Schisano, E., Giannini, T., Hill, T., Lorenzetti, D., Menten, K., Olmi, L., Schuller, F., Strafella, F., De Luca, M., Motte, F., Wyrowski, F.
Publikováno v:
A&A 628, A110 (2019)
Context The Vela Molecular Ridge is one of the nearest (700 pc) giant molecular cloud (GMC) complexes hosting intermediate-mass (up to early B, late O stars) star formation, and is located in the outer Galaxy, inside the Galactic plane. Vela C is one
Externí odkaz:
http://arxiv.org/abs/1907.07609
Autor:
Strack, A., Araya, E. D., Lebrón, M. E., Minchin, R. F., Arce, H. G., Ghosh, T., Hofner, P., Kurtz, S., Olmi, L., Pihlström, Y., Salter, C. J.
Publikováno v:
2019 ApJ 878 90
Jets and outflows are ubiquitous phenomena in astrophysics, found in our Galaxy in diverse environments, from the formation of stars to late-type stellar objects. We present observations conducted with the 305m Arecibo Telescope of the pre-planetary
Externí odkaz:
http://arxiv.org/abs/1906.08245
Autor:
Andreev, N., Araya, E. D., Hoffman, I. M., Hofner, P., Kurtz, S., Linz, H., Olmi, L., Lorran-Costa, I.
We present results of a multi-epoch monitoring program on variability of 6$\,$cm formaldehyde (H$_2$CO) masers in the massive star forming region NGC$\,$7538$\,$IRS$\,$1 from 2008 to 2015 conducted with the GBT, WSRT, and VLA. We found that the simil
Externí odkaz:
http://arxiv.org/abs/1709.02903