Zobrazeno 1 - 10
of 972
pro vyhledávání: '"Lees R"'
Autor:
Ilyushin, V. V., Müller, H. S. P., Drozdovskaya, M. N., Jørgensen, J. K., Bauerecker, S., Maul, C., Porohovoi, R., Alekseev, E. A., Dorovskaya, O., Zakharenko, O., Lewen, F., Schlemmer, S., Lees, R. M.
We have started a measurement campaign of numerous methanol isotopologs in low-lying torsional states in order to provide extensive line lists for radio astronomical observations from an adequate spectroscopic model and to investigate how the intrica
Externí odkaz:
http://arxiv.org/abs/2406.08236
Autor:
Ilyushin, V. V., Müller, H. S. P., Jørgensen, J. K., Bauerecker, S., Maul, C., Porohovoi, R., Alekseev, E. A., Dorovskaya, O., Lewen, F., Schlemmer, S., Lees, R. M.
Publikováno v:
A&A 677, A49 (2023)
Solar-type prestellar cores and protostars display large amounts of deuterated organic molecules. Recent findings on CHD$_2$OH and CD$_3$OH toward IRAS 16293-2422 suggest that even fully deuterated methanol, CD$_3$OD, may be detectable as well. Howev
Externí odkaz:
http://arxiv.org/abs/2307.07801
Autor:
Ranaivomanana, P., Johnston, C., Groot, P. J., Aerts, C., Lees, R., IJspeert, L., Bloemen, S., Klein-Wolt, M., Woudt, P., Kording, E., Poole, R. Le, Pieterse, D.
Publikováno v:
A&A 672, A69 (2023)
Colour-magnitude diagrams reveal a population of blue (hot) sub-luminous objects with respect to the main sequence. These hot sub-luminous stars are the result of evolutionary processes that require stars to expel their obscuring, hydrogen-rich envel
Externí odkaz:
http://arxiv.org/abs/2302.07266
Autor:
Lee, H. -J., Kim, M. -J., Marciniak, A., Kim, D. -H., Moon, H. -K., Choi, Y. -J., Zoła, S., Chatelain, J., Lister, T. A., Gomez, E., Greenstreet, S., Pál, A., Szakáts, R., Erasmus, N., Lees, R., van Rensburg, P. Janse, Ogłoza, W., Dróżdż, M., Żejmo, M., Kamiński, K., Kamińska, M. K., Duffard, R., Roh, D. -G., Yim, H. -S., Kim, T., Mottola, S., Yoshida, F., Reichart, D. E., Sonbas, E., Caton, D. B., Kaplan, M., Erece, O., Yang, H.
Publikováno v:
A&A 661, L3 (2022)
Context. The close approach of the near-Earth asteroid (99942) Apophis to Earth in 2029 will provide a unique opportunity to examine how the physical properties of the asteroid could be changed due to the Earth's gravitational perturbation. As a resu
Externí odkaz:
http://arxiv.org/abs/2204.02540
Autor:
Ilyushin, V. V., Müller, H. S. P., Jørgensen, J. K., Bauerecker, S., Maul, C., Bakhmat, Y., Alekseev, E. A., Dorovskaya, O., Vlasenko, S., Lewen, F., Schlemmer, S., Berezkin, K., Lees, R. M.
Publikováno v:
A&A 658, A127 (2022)
Solar-type protostars harbor highly deuterated complex organics. While this degree of deuteration may provide important clues in studying the formation of these species, spectroscopic information on multiply deuterated isotopologs is often insufficie
Externí odkaz:
http://arxiv.org/abs/2111.09055
Autor:
Xu, Li-Hong, Lees, R. M., Zakharenko, O., Müller, H. S. P., Lewen, F., Schlemmer, S., Menten, K. M.
Publikováno v:
J. Mol. Spectrosc. 378 (2021) 111473
The dramatic increase in sensitivity, spectral coverage and resolution of radio astronomical facilities in recent years has opened new possibilities for observation of chemical differentiation and isotopic fractionation in protostellar sources to she
Externí odkaz:
http://arxiv.org/abs/2104.14340
Autor:
Ilyushin, V. V., Zakharenko, O., Lewen, F., Schlemmer, S., Alekseev, E. A., Pogrebnyak, M., Lees, R. M., Xu, L. -H., Belloche, A., Menten, K. M., Garrod, R. T., Müller, H. S. P.
Publikováno v:
Can. J. Phys. 98 (2020) 530-537
Methyl mercaptan (CH3SH) is a known interstellar molecule with abundances high enough that the detection of some of its minor isotopologues is promising. The present study aims at providing accurate spectroscopic parameters for the (13)CH3SH isotopol
Externí odkaz:
http://arxiv.org/abs/1910.02259
Autor:
Zakharenko, O., Ilyushin, V. V., Lewen, F., Müller, H. S. P., Schlemmer, S., Alekseev, E. A., Pogrebnyak, M. L., Armieieva, I. A., Dorovskaya, O., Xu, L. -H., Lees, R. M.
Publikováno v:
A&A 629, A73 (2019)
We present a new global study of the millimeter (mm) wave, submillimeter (sub-mm) wave, and terahertz (THz) spectra of the lowest three torsional states of methyl mercaptan (CH$_3$SH). New measurements have been carried out between 50 and 510 GHz usi
Externí odkaz:
http://arxiv.org/abs/1908.07790
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Borissova, A., Soni, S., Aston, E.R., Lees, R., Petrilli, K., Wall, M.B., Bloomfield, M.A.P., Mertzani, E., Paksina, A., Freeman, T.P., Mokrysz, C., Lawn, W., Curran, H.V.
Publikováno v:
In Drug and Alcohol Dependence 1 September 2022 238