Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Surina, F."'
Autor:
Mueangkon, Y., Khamrat, S., Suekong, D., Aintawiphak, S., Jaiboe, A., Surina, F., Darnley, M. J., Bode, M. F.
Publikováno v:
Mueangkon et al 2018 J. Phys.: Conf. Ser. 1144 012014
We study the evolution of V339 Del (Nova Del 2013) during 0.37 to 75 days after discovery. Spectra from the Liverpool Telescope were collected and analysed to find velocity of ejecta, relative radiation with respect to continuum level, and FWHM of th
Externí odkaz:
http://arxiv.org/abs/1812.10871
Autor:
Hounsell, R., Darnley, M. J., Bode, M. F., Harman, D. J., Surina, F., Starrfield, S., Holdsworth, D. L., Bewsher, D., Hick, P. P., Jackson, B. V., Buffington, A., Clover, J. M., Shafter, A. W.
We present the results from observing nine Galactic novae in eruption with the Solar Mass Ejection Imager (SMEI) between 2004 and 2009. While many of these novae reached peak magnitudes that were either at or approaching the detection limits of SMEI,
Externí odkaz:
http://arxiv.org/abs/1512.03321
We investigated the optical lightcurve of T Pyx during its 2011 outburst by compiling a database of SMEI and AAVSO observations. The SMEI lightcurve, providing unprecedented detail covering 1.5-49d post-discovery, was divided into four phases based o
Externí odkaz:
http://arxiv.org/abs/1402.1109
Autor:
Khamrat, S., Noysena, K., Surina, F., Ackley, K., Dyer, M. J., Jiménez-Ibarra, F., Lyman, J., Ulaczyk, K., Steeghs, D., Galloway, D. K., Dhillon, V. S., O'Brien, P., Ramsay, G., Kotak, R., Breton, R. P., Nuttall, L. K., Pall'e, E., Pollacco, D., Killestein, T., Kumar, A.
Publikováno v:
ASP Conference Series; 2024, Vol. 536, p35-40, 6p
We investigated the optical light curve of T Pyx during its 2011 outburst through compiling a database of SMEI and AAVSO observations. The SMEI light curve, providing unprecedented detail with high cadence data during t=1.5-49 days post-discovery, wa
Externí odkaz:
http://arxiv.org/abs/1303.6592
Autor:
Darnley, M. J., Bode, M. F., Harman, D. J., Hounsell, R. A., Munari, U., Ribeiro, V. A. R. M., Surina, F., Williams, R. P., Williams, S. C.
Of the 350 or more known Galactic classical novae, only a handful of them, the recurrent novae, have been observed in outburst more than once. At least eight of these recurrents are known to harbour evolved secondary stars, rather than the main seque
Externí odkaz:
http://arxiv.org/abs/1303.2711
Publikováno v:
Journal of Physics: Conference Series; Nov2023, Vol. 2653 Issue 1, p1-10, 10p
Autor:
Surina, F
Classical novae (CNe) are interacting binary systems whose outbursts are powered by a thermonuclear runaway in accreted material on the surface of a white dwarf (WD). The secondary stars in such systems fill their Roche lobe and material is transferr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d32e5766b9578deb4687fb495b791f7b
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