Standard

A 3-D look into the atmosphere? / Wade, G. A.; Mashonkina, L.; Ryabchikova, T.; Krticka, J.; Silvester, J.; Kochukhov, O.; Sousa, J. C.; Nomura, T.; Wahlgren, G. M.; Gruberbauer, M.; Hubrig, S.; Briquet, M.; Yuce, K.; Drake, N.; Nunez, N.; Gray, R. O.; Ziznovsky, J.; Cowley, C.; Shavrina, A.; Dworetsky, M.

In: Proceedings of the International Astronomical Union, 2010, p. 151-160.

Research output: Contribution to journal › Article › peer-review

Harvard

Wade, GA, Mashonkina, L, Ryabchikova, T, Krticka, J, Silvester, J, Kochukhov, O, Sousa, JC, Nomura, T, Wahlgren, GM, Gruberbauer, M, Hubrig, S, Briquet, M, Yuce, K, Drake, N, Nunez, N, Gray, RO, Ziznovsky, J, Cowley, C, Shavrina, A & Dworetsky, M 2010, 'A 3-D look into the atmosphere?', Proceedings of the International Astronomical Union, pp. 151-160. https://doi.org/10.1017/S1743921310008550

APA

Wade, G. A., Mashonkina, L., Ryabchikova, T., Krticka, J., Silvester, J., Kochukhov, O., Sousa, J. C., Nomura, T., Wahlgren, G. M., Gruberbauer, M., Hubrig, S., Briquet, M., Yuce, K., Drake, N., Nunez, N., Gray, R. O., Ziznovsky, J., Cowley, C., Shavrina, A., & Dworetsky, M. (2010). A 3-D look into the atmosphere? Proceedings of the International Astronomical Union, 151-160. https://doi.org/10.1017/S1743921310008550

Vancouver

Wade GA, Mashonkina L, Ryabchikova T, Krticka J, Silvester J, Kochukhov O et al. A 3-D look into the atmosphere? Proceedings of the International Astronomical Union. 2010;151-160. https://doi.org/10.1017/S1743921310008550

Author

Wade, G. A. ; Mashonkina, L. ; Ryabchikova, T. ; Krticka, J. ; Silvester, J. ; Kochukhov, O. ; Sousa, J. C. ; Nomura, T. ; Wahlgren, G. M. ; Gruberbauer, M. ; Hubrig, S. ; Briquet, M. ; Yuce, K. ; Drake, N. ; Nunez, N. ; Gray, R. O. ; Ziznovsky, J. ; Cowley, C. ; Shavrina, A. ; Dworetsky, M. / A 3-D look into the atmosphere?. In: Proceedings of the International Astronomical Union. 2010 ; pp. 151-160.

BibTeX

@article{112ef1049c6141f18a701d70986c2fc2,
title = "A 3-D look into the atmosphere?",
abstract = "The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an important window to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session “A 3D look into the atmosphere” of the Joint Discussion “Progress in understanding the physics of Ap and related stars”. It is divided into 3 sections: “Magnetic field and surface structures”, “Pulsations in the atmospheres of roAp stars/inversions”, and “Spectral synthesis/atmospheric models”.",
keywords = "stars: chemically peculiar, stars: atmospheres, stars: variables: roAp stars, stars: magnetic fields",
author = "Wade, {G. A.} and L. Mashonkina and T. Ryabchikova and J. Krticka and J. Silvester and O. Kochukhov and Sousa, {J. C.} and T. Nomura and Wahlgren, {G. M.} and M. Gruberbauer and S. Hubrig and M. Briquet and K. Yuce and N. Drake and N. Nunez and Gray, {R. O.} and J. Ziznovsky and C. Cowley and A. Shavrina and M. Dworetsky",
year = "2010",
doi = "10.1017/S1743921310008550",
language = "English",
pages = "151--160",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",

}

RIS

TY - JOUR

T1 - A 3-D look into the atmosphere?

AU - Wade, G. A.

AU - Mashonkina, L.

AU - Ryabchikova, T.

AU - Krticka, J.

AU - Silvester, J.

AU - Kochukhov, O.

AU - Sousa, J. C.

AU - Nomura, T.

AU - Wahlgren, G. M.

AU - Gruberbauer, M.

AU - Hubrig, S.

AU - Briquet, M.

AU - Yuce, K.

AU - Drake, N.

AU - Nunez, N.

AU - Gray, R. O.

AU - Ziznovsky, J.

AU - Cowley, C.

AU - Shavrina, A.

AU - Dworetsky, M.

PY - 2010

Y1 - 2010

N2 - The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an important window to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session “A 3D look into the atmosphere” of the Joint Discussion “Progress in understanding the physics of Ap and related stars”. It is divided into 3 sections: “Magnetic field and surface structures”, “Pulsations in the atmospheres of roAp stars/inversions”, and “Spectral synthesis/atmospheric models”.

AB - The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In addition to providing an important window to understanding the physical processes at play in these complex atmospheres, they can also be exploited to study stellar pulsations. This article reviews contributions to the session “A 3D look into the atmosphere” of the Joint Discussion “Progress in understanding the physics of Ap and related stars”. It is divided into 3 sections: “Magnetic field and surface structures”, “Pulsations in the atmospheres of roAp stars/inversions”, and “Spectral synthesis/atmospheric models”.

KW - stars: chemically peculiar

KW - stars: atmospheres

KW - stars: variables: roAp stars

KW - stars: magnetic fields

U2 - 10.1017/S1743921310008550

DO - 10.1017/S1743921310008550

M3 - Article

SP - 151

EP - 160

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -

ID: 5391365