Standard
SIO MASER MOVIES: THE RE-RUN. / Gray, M. D.; Wittkowski, M.; Humphreys, E. M. L. и др.
в:
Труды Института прикладной астрономии РАН, № 40, 2017, стр. 78-83.
Результаты исследований: Вклад в журнал › Статья › Рецензирование
Harvard
Gray, MD, Wittkowski, M, Humphreys, EML
, Parfenov, SY & Sobolev, M 2017, '
SIO MASER MOVIES: THE RE-RUN',
Труды Института прикладной астрономии РАН, № 40, стр. 78-83.
APA
Gray, M. D., Wittkowski, M., Humphreys, E. M. L.
, Parfenov, S. Y., & Sobolev, M. (2017).
SIO MASER MOVIES: THE RE-RUN.
Труды Института прикладной астрономии РАН, (40), 78-83.
Vancouver
Author
Gray, M. D. ; Wittkowski, M. ; Humphreys, E. M. L. и др. /
SIO MASER MOVIES: THE RE-RUN. в:
Труды Института прикладной астрономии РАН. 2017 ; № 40. стр. 78-83.
BibTeX
@article{b79fdb9e04ee4dacbd3a76454b30354e,
title = "SIO MASER MOVIES: THE RE-RUN",
abstract = "We report preliminary results of a new time-dependent model of SiO maser emission in the extended atmosphere of an AGB star. We compare this model to time-series observations of SiO masers towards the Mira variable TX Cam. The model masers are predominantly radiatively pumped, at least in the second half of the stellar pulsation period. Predictions for the radius of peak maser brightness and the width of the maser ring are broadly in line with the observations.",
author = "Gray, {M. D.} and M. Wittkowski and Humphreys, {E. M. L.} and Parfenov, {S. Yu.} and M. Sobolev",
year = "2017",
language = "English",
pages = "78--83",
journal = "Труды Института прикладной астрономии РАН",
issn = "2224-7440",
publisher = "Институт прикладной астрономии Российской академии наук",
number = "40",
}
RIS
TY - JOUR
T1 - SIO MASER MOVIES: THE RE-RUN
AU - Gray, M. D.
AU - Wittkowski, M.
AU - Humphreys, E. M. L.
AU - Parfenov, S. Yu.
AU - Sobolev, M.
PY - 2017
Y1 - 2017
N2 - We report preliminary results of a new time-dependent model of SiO maser emission in the extended atmosphere of an AGB star. We compare this model to time-series observations of SiO masers towards the Mira variable TX Cam. The model masers are predominantly radiatively pumped, at least in the second half of the stellar pulsation period. Predictions for the radius of peak maser brightness and the width of the maser ring are broadly in line with the observations.
AB - We report preliminary results of a new time-dependent model of SiO maser emission in the extended atmosphere of an AGB star. We compare this model to time-series observations of SiO masers towards the Mira variable TX Cam. The model masers are predominantly radiatively pumped, at least in the second half of the stellar pulsation period. Predictions for the radius of peak maser brightness and the width of the maser ring are broadly in line with the observations.
UR - https://elibrary.ru/item.asp?id=32446282
M3 - Article
SP - 78
EP - 83
JO - Труды Института прикладной астрономии РАН
JF - Труды Института прикладной астрономии РАН
SN - 2224-7440
IS - 40
ER -
