Zobrazeno 1 - 10
of 300
pro vyhledávání: '"Tamassia, F"'
Autor:
Melosso, M., Bizzocchi, L., Adamczyk, A., Canè, E., Caselli, P., Colzi, L., Dore, L., Giuliano, B. M., Guillemin, J. -C., Martin-Drumel, M. -A., Pirali, O., Charmet, A. Pietropolli, Prudenzano, D., Rivilla, V. M., Tamassia, F.
Cyanoacetylene, the simplest cyanopolyyne, is an abundant interstellar molecule commonly observed in a vast variety of astronomical sources. Despite its importance as a potential tracer of the evolution of star-forming processes, the deuterated form
Externí odkaz:
http://arxiv.org/abs/2007.09995
Autor:
Lamperti, M., Gotti, R., Gatti, D., Shakfa, M. K., Cané, E., Tamassia, F., Schunemann, P., Laporta, P., Farooq, A., Marangoni, M.
Publikováno v:
Commun Phys 3, 175 (2020)
Frequency combs have triggered an impressive evolution of optical metrology across diverse regions of the electromagnetic spectrum, from the ultraviolet to the terahertz frequencies. An unexplored territory, however, remains in the region of vibratio
Externí odkaz:
http://arxiv.org/abs/2007.08257
Autor:
Melosso, M., Bizzocchi, L., Sipilä, O., Giuliano, B. M., Dore, L., Tamassia, F., Martin-Drumel, M. -A., Pirali, O., Redaelli, E., Caselli, P.
Publikováno v:
A&A 641, A153 (2020)
Deuterium fractionation processes in the interstellar medium (ISM) have been shown to be highly efficient in the family of nitrogen hydrides. To date, observations were limited to ammonia (NH$_2$D, NHD$_2$, ND$_3$) and imidogen radical (ND) isotopolo
Externí odkaz:
http://arxiv.org/abs/2007.07504
Autor:
Melosso, M., Achilli, A., Tamassia, F., Canè, E., Charmet, A. Pietropolli, Stoppa, P., Dore, L.
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 248, June 2020, 106982
Chloromethane is the only organochloride detected in space to date. Its recent observation towards the low-mass protostar IRAS 16293-2422 with ALMA offers a prompt for new laboratory studies of CH$_3$Cl and its isotopologues. Here, we report the inve
Externí odkaz:
http://arxiv.org/abs/2006.13676
Autor:
Melosso, M., Belloche, A., Martin-Drumel, M. -A., Pirali, O., Tamassia, F., Bizzocchi, L., Garrod, R. T., Müller, H. S. P., Menten, K. M., Dore, L., Puzzarini, C.
Publikováno v:
A&A 641, A160 (2020)
Aminoacetonitrile, a molecule detected in the interstellar medium only towards the star-forming region Sagittarius B2 (Sgr B2) thus far, is considered an important prebiotic species. To date, observations were limited to ground state emission lines,
Externí odkaz:
http://arxiv.org/abs/2006.13753
Autor:
Rivilla, V. M., Colzi, L., Fontani, F., Melosso, M., Caselli, P., Bizzocchi, L., Tamassia, F., Dore, L.
We present the study of deuteration of cyanoacetylene (HC$_3$N) towards a sample of 28 high-mass star-forming cores divided into different evolutionary stages, from starless to evolved protostellar cores. We report for the first time the detection of
Externí odkaz:
http://arxiv.org/abs/2005.14118
Autor:
Gordon, I.E., Rothman, L.S., Hargreaves, R.J., Hashemi, R., Karlovets, E.V., Skinner, F.M., Conway, E.K., Hill, C., Kochanov, R.V., Tan, Y., Wcisło, P., Finenko, A.A., Nelson, K., Bernath, P.F., Birk, M., Boudon, V., Campargue, A., Chance, K.V., Coustenis, A., Drouin, B.J., Flaud, J.–M., Gamache, R.R., Hodges, J.T., Jacquemart, D., Mlawer, E.J., Nikitin, A.V., Perevalov, V.I., Rotger, M., Tennyson, J., Toon, G.C., Tran, H., Tyuterev, V.G., Adkins, E.M., Baker, A., Barbe, A., Canè, E., Császár, A.G., Dudaryonok, A., Egorov, O., Fleisher, A.J., Fleurbaey, H., Foltynowicz, A., Furtenbacher, T., Harrison, J.J., Hartmann, J.–M., Horneman, V.–M., Huang, X., Karman, T., Karns, J., Kassi, S., Kleiner, I., Kofman, V., Kwabia–Tchana, F., Lavrentieva, N.N., Lee, T.J., Long, D.A., Lukashevskaya, A.A., Lyulin, O.M., Makhnev, V.Yu., Matt, W., Massie, S.T., Melosso, M., Mikhailenko, S.N., Mondelain, D., Müller, H.S.P., Naumenko, O.V., Perrin, A., Polyansky, O.L., Raddaoui, E., Raston, P.L., Reed, Z.D., Rey, M., Richard, C., Tóbiás, R., Sadiek, I., Schwenke, D.W., Starikova, E., Sung, K., Tamassia, F., Tashkun, S.A., Vander Auwera, J., Vasilenko, I.A., Vigasin, A.A., Villanueva, G.L., Vispoel, B., Wagner, G., Yachmenev, A., Yurchenko, S.N.
Publikováno v:
In Journal of Quantitative Spectroscopy and Radiative Transfer January 2022 277
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Autor:
Tamassia, F., Bizzocchi, L., Melosso, M., Martin-Drumel, M. -A., Pirali, O., Pietropolli Charmet, A., Cane, E., Dore, L., Gordon, I. E., Guillemin, J. -C., Giuliano, B. M., Caselli, P., Alessandrini, S., Barone, V., Puzzarini, C.
The far-infrared spectrum of HC3N has been recorded at high resolution between 70 and 500 cm−1using synchrotron radiation. Four prominent features, i.e., ν7, ν6−ν7, ν4−ν6, and 2ν7 have been identified in the spectrum together with many as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::cc9c47306b37e4d41cf65154cc50fb41
https://hdl.handle.net/11585/872019
https://hdl.handle.net/11585/872019