Zobrazeno 1 - 10
of 193
pro vyhledávání: '"Gabriele Cazzoli"'
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 168:10-16
The investigation of the pure rotational spectrum of the 17O2 isotopic species of molecular oxygen has been extended with respect to previous investigations to the submillimeter-wave region, from 230 GHz up to 1.06 THz. The resulting spectroscopic pa
Autor:
Gabriele Cazzoli, Jürgen Gauss, Valerio Lattanzi, Cristina Puzzarini, Sonia Coriani, José Cernicharo, Claudio Codella, Andrés Asensio Ramos
Publikováno v:
Proceedings of the 72nd International Symposium on Molecular Spectroscopy.
Magnetic fields play a fundamental role in star formation processes and the best method to evaluate their intensity is is to measure the Zeeman effect of atomic and molecular lines. However, a direct measurement of the Zeeman spectral pattern from in
Autor:
Cristina Puzzarini, Gabriele Cazzoli
Publikováno v:
The Journal of Physical Chemistry A. 119:1765-1773
Methyl fluoride is a prototypical symmetric-top molecule. Despite the fact that its rotational spectrum has been largely investigated, centrifugal-distortion constants were determined only up to the sextic terms. The present investigation demonstrate
Autor:
Cristina Puzzarini, Gabriele Cazzoli
Publikováno v:
Journal of Molecular Spectroscopy. 298:31-37
The rotational spectra of two isotopic species of hydrogen sulfide have been revisited. For H 2 33 S, which was detected in natural abundance, accurate measurements were performed in the submillimeter-wave region, from 500 GHz up to 1.56 THz, thus al
Autor:
Cristina Puzzarini, Jürgen Gauss, Andrés Asensio Ramos, Gabriele Cazzoli, Claudio Codella, Valerio Lattanzi, José Cernicharo, Sonia Coriani
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Coriani, S, Cazzoli, G, Lattanzi, V, Gauss, J, Codella, C, Asensio Ramos, A, Cernicharo, J & Puzzarini, C 2017, ' Zeeman effect in sulfur monoxide : a tool to probe magnetic fields in star forming regions ', Astronomy & Astrophysics, vol. 605, A20 . https://doi.org/10.1051/0004-6361/201730858
Cazzoli, G, Lattanzi, V, Coriani, S, Gauss, J, Codella, C, Ramos, A A, Cernicharo, J & Puzzarini, C 2017, ' Zeeman effect in sulfur monoxide: a tool to probe magnetic fields in star forming regions ', Astronomy and Astrophysics, vol. 605, A20 . https://doi.org/10.1051/0004-6361/201730858
instname
Coriani, S, Cazzoli, G, Lattanzi, V, Gauss, J, Codella, C, Asensio Ramos, A, Cernicharo, J & Puzzarini, C 2017, ' Zeeman effect in sulfur monoxide : a tool to probe magnetic fields in star forming regions ', Astronomy & Astrophysics, vol. 605, A20 . https://doi.org/10.1051/0004-6361/201730858
Cazzoli, G, Lattanzi, V, Coriani, S, Gauss, J, Codella, C, Ramos, A A, Cernicharo, J & Puzzarini, C 2017, ' Zeeman effect in sulfur monoxide: a tool to probe magnetic fields in star forming regions ', Astronomy and Astrophysics, vol. 605, A20 . https://doi.org/10.1051/0004-6361/201730858
[Context] Magnetic fields play a fundamental role in star formation processes and the best method to evaluate their intensity is to measure the Zeeman effect of atomic and molecular lines. However, a direct measurement of the Zeeman spectral pattern
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::174f4bdd3e42d5fe2d93ad6aa18808d9
http://hdl.handle.net/11585/624727
http://hdl.handle.net/11585/624727
Autor:
Cristina Puzzarini, Gabriele Cazzoli
Publikováno v:
Proceedings of the 71st International Symposium on Molecular Spectroscopy.
Publikováno v:
Proceedings of the 71st International Symposium on Molecular Spectroscopy.
Publikováno v:
Molecular Physics
Molecular Physics, Taylor & Francis, 2011, 109 (17-18), pp.1-5. ⟨10.1080/00268976.2011.609142⟩
Molecular Physics, Taylor & Francis, 2011, 109 (17-18), pp.1-5. ⟨10.1080/00268976.2011.609142⟩
International audience; The rotational spectrum of fluoroiodomethane, CH2FI, has been recorded in the 1.02-1.05 THz frequency range, allowing to extend the set of known spectroscopic parameters with respect to our previous work [J. Chem. Phys. 134, 1
Publikováno v:
Journal of Molecular Spectroscopy. 267:118-122
We have used the theoretical predictions from anharmonic force field calculations reported in our previous work [J. Mol. Spectrosc. 253 (2009) 106] to assign the pure rotational spectra in the v 12 and v 13 doubly degenerate bending modes of the main
Publikováno v:
Astronomy & Astrophysics. 507:1707-1710
The ground-state inversion-rotation transition of ammonia at 572.498 GHz has been investigated in the laboratory using a sourcemodulation microwave spectrometer equipped with a double-pass cell. The experiment has been carried out at a pressure lower