Zobrazeno 1 - 10
of 1 566
pro vyhledávání: '"Gray, M D"'
We use 3D computer modelling to investigate the timescales and radiative output from maser flares generated by the impact of shock-waves on astronomical unit-scale clouds in interstellar and star-forming regions, and in circumstellar regions in some
Externí odkaz:
http://arxiv.org/abs/2404.10741
Publikováno v:
Proceedings of the Academy of Natural Sciences of Philadelphia, 1854 Jan 01. 7, 423-454.
Externí odkaz:
https://www.jstor.org/stable/4059092
Autor:
Gray, Edward Whitaker
Publikováno v:
Philosophical Transactions of the Royal Society of London, 1788 Jan 01. 78, 121-124.
Externí odkaz:
https://www.jstor.org/stable/106651
Autor:
Gray, Edward Whitaker
Publikováno v:
Philosophical Transactions of the Royal Society of London, 1789 Jan 01. 79, 21-36.
Externí odkaz:
https://www.jstor.org/stable/106678
Autor:
Wilson, Giffin, Gray, Edward Whitaker
Publikováno v:
Philosophical Transactions of the Royal Society of London, 1799 Jan 01. 89, 265-304.
Externí odkaz:
https://www.jstor.org/stable/107037
Autor:
Gray, Edward Whitaker
Publikováno v:
Philosophical Transactions of the Royal Society of London, 1796 Jan 01. 86, 353-381.
Externí odkaz:
https://www.jstor.org/stable/107010
Autor:
Young, Thomas
Publikováno v:
Philosophical Transactions of the Royal Society of London, 1800 Jan 01. 90, 106-150.
Externí odkaz:
https://www.jstor.org/stable/107049
ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited H$_2$O and OH lines
Autor:
Baudry, A., Wong, K. T., Etoka, S., Richards, A. M. S., Muller, H. S. P., Herpin, F., Danilovich, T., Gray, M. D., Wallstrom, S., Gobrecht, D., Khouri, T., Decin, L., Gottlieb, C. A., Menten, K. M., Homan, W., Millar, T. J., Montarges, M., Pimpanuwat, B., Plane, J. M. C., Kervella, P.
Publikováno v:
A&A 674, A125 (2023)
Water and the hydroxyl radical are major constituents of the envelope of O-rich late-type stars. Transitions involving energy levels that are highly excited have been observed in both H$_2$O and OH. These and more recently discovered transitions can
Externí odkaz:
http://arxiv.org/abs/2305.03171
Autor:
Montargès, M., Cannon, E., de Koter, A., Khouri, T., Lagadec, E., Kervella, P., Decin, L., McDonald, I., Homan, W., Waters, L. B. F. M., Sahai, R., Gottlieb, C. A., Malfait, J., Maes, S., Pimpanuwat, B., Jeste, M., Danilovich, T., De Ceuster, F., Van de Sande, M., Gobrecht, D., Wallström, S. H. J., Wong, K. T., Mellah, I. El, Bolte, J., Herpin, F., Richards, A. M. S., Baudry, A., Etoka, S., Gray, M. D., Millar, T. J., Menten, K. M., Müller, H. S. P., Plane, J. M. C., Yates, J., Zijlstra, A.
Publikováno v:
A&A 671, A96 (2023)
Aims. Through the ATOMIUM project, based on an ALMA large program, we aim to present a consistent view of a sample of 17 nearby cool evolved stars (Aymptotic Giant Branch and red supergiant stars). Methods. Here we present VLT/SPHERE-ZIMPOL polarimet
Externí odkaz:
http://arxiv.org/abs/2301.02081
Autor:
Evans, A., Pimpanuwat, B., Richards, A. M. S., Banerjee, D. P. K., Munari, U., Gray, M. D., Kramer, B. Hutawarakorn, Kraus, A.
Publikováno v:
MNRAS, 514, 4894 - 4897 (2022)
There are indications that the third known eruption of the recurrent nova T CrB is imminent, and multi-wavelength observations prior to the eruption are important to characterise the system before it erupts. T CrB is known to display the SiO fundamen
Externí odkaz:
http://arxiv.org/abs/2207.14743