| Форма представления | Статьи в зарубежных журналах и сборниках |
| Год публикации | 2017 |
| Язык | английский |
|
Шиманский Владислав Владимирович, автор
|
| Библиографическое описание на языке оригинала |
Galazutdinov C.A. C+60 – looking for the bucky-ball in interstellar space / G.A. Galazutdinov, V.V. Shimansky, A. Bondar, G. Valyavin, J. Krełowski // MNRAS. -2017. - V.465. - P.3956–3964. |
| Аннотация |
MNRAS |
| Ключевые слова |
ISM: clouds, ISM: lines and bands, ISM: molecules. |
| Название журнала |
MNRAS
|
| Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=151691 |
Полная запись метаданных  |
| Поле DC |
Значение |
Язык |
| dc.contributor.author |
Шиманский Владислав Владимирович |
ru_RU |
| dc.date.accessioned |
2017-01-01T00:00:00Z |
ru_RU |
| dc.date.available |
2017-01-01T00:00:00Z |
ru_RU |
| dc.date.issued |
2017 |
ru_RU |
| dc.identifier.citation |
Galazutdinov C.A. C+60 – looking for the bucky-ball in interstellar space / G.A. Galazutdinov, V.V. Shimansky, A. Bondar, G. Valyavin, J. Krełowski // MNRAS. -2017. - V.465. - P.3956–3964. |
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/?p_id=151691 |
ru_RU |
| dc.description.abstract |
MNRAS |
ru_RU |
| dc.description.abstract |
The laboratory gas-phase spectrum recently published by Campbell et al. has reinvigorated attempts to confirm the presence of the C+60 cation in the interstellar medium, through an analysis of the spectra of hot, reddened stars. This search is hindered by at least two issues that need to be addressed: (i) the wavelength range of interest is severely polluted by strong water-vapour lines coming from the Earth's atmosphere; (ii) one of the major bands attributed to C+60, at 9633 Å, is blended with the stellar MgII line, which is susceptible to non-local thermodynamic equilibrium effects in hot stellar atmospheres. Both these issues are carefully considered here for the first time, based on high-resolution and high signal-to-noise ratio echell´e spectra for 19 lines of sight. The result is that the presence of C+60 in interstellar clouds is brought into question. |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
ISM: clouds |
ru_RU |
| dc.subject |
ISM: lines and bands |
ru_RU |
| dc.subject |
ISM: molecules. |
ru_RU |
| dc.title |
C+60 – looking for the bucky-ball in interstellar space |
ru_RU |
| dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|
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