Zobrazeno 1 - 10
of 473
pro vyhledávání: '"Felli M."'
Publikováno v:
In Transportation Research Procedia 2023 72:1958-1965
Publikováno v:
In European Journal of Mechanics / B Fluids January-February 2019 73:24-47
Akademický článek
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Autor:
Felli, M., Brand, J., Cesaroni, R., Codella, C., Comoretto, G., Di Franco, S., Massi, F., Moscadelli, L., Nesti, R., Olmi, L., Palagi, F., Panella, D., Valdettaro, R.
Context. Water vapor emission at 22 GHz from masers associated with star-forming regions is highly variable. Aims. We present a database of up to 20 years of monitoring of a sample of 43 masers within star-forming regions. The sample covers a large r
Externí odkaz:
http://arxiv.org/abs/0710.0790
Publikováno v:
Astrophys.Space Sci. 295 (2005) 133-141
An overview is given of the analysis of more than a decade of H2O maser data from our monitoring program. We find the maser emission to generally depend on the luminosity of the YSO as well as on the geometry of the SFR. There appears to be a thresho
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407217
Publikováno v:
Astron.Astrophys. 420 (2004) 553-569
The S235A-B star forming region has been extensively observed in the past from the radio to the near-IR, but what was happening in the immediate surroundings of the water maser, placed in between the two nebulosities, was still unclear because of ins
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403483
Publikováno v:
Astron.Astrophys. 407 (2003) 573-588
(Abridged) H2O masers in 14 SFRs have been monitored once every 2-3 months for up to 13 years. We investigate the dependence of the overall spectral morphology of the maser emission and its variability on the luminosity of the YSO, and look for burst
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306249
Autor:
Omont, A., Gilmore, G., Alard, C., Aracil, B., August, T., Baliyan, K., Blommaert, J., Borsenberger, J., Burgdorf, M., Cesarsky, C., de Batz, B., Egan, M., Egret, D., Epchtein, N., Felli, M., Fouque, P., Ganesh, S., Glass, I., Gredel, R., Groenewegen, M., Habing, H. J., Hennebelle, P., Jiang, B., Joshi, U., Messineo, M., Miville-Deschenes, M. A., Moneti, A., Ojha, D., Ortiz, R., Ott, S., Perault, M., Price, S., Robin, A., Schultheis, M., Schuller, F., Simon, G., Testi, L., Teyssier, D., van Loon, J., Wyse, R.
Publikováno v:
Astron.Astrophys. 403 (2003) 975-992
The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss and the recent star formation history of the inner disk and Bulge of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304383
The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by IRAS because of lower sensitivity or confusion probl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0207058
Autor:
Alard, C., Blommaert, J., Cesarsky, C., Epchtein, N., Felli, M., Fouque, P., Ganesh, S., Genzel, R., Gilmore, G., Glass, I., Habing, H., Omont, A., Perault, M., Price, S., Robin, A., Schultheis, M., Simon, G., van Loon, J., Alcock, C., Allsman, R., Alves, D., Axelrod, T., Becker, A., Bennett, D., Cook, K., Drake, A., Freeman, K., Geha, M., Griest, K., Lehner, M., Marshall, S., Minniti, D., Nelson, C., Peterson, B., Popowski, P., Pratt, M., Quinn, P., Sutherland, W., Tomaney, A., Vandehei, T., Welch, D.
By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been determined. ISOGAL mid-infrared photometry and MACHO lightcurves are assembled for approximat
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101094