Zobrazeno 1 - 10
of 246
pro vyhledávání: '"Aungwerojwit, A."'
Autor:
Robert, Akshay, Farihi, Jay, Van Eylen, Vincent, Aungwerojwit, Amornrat, Gänsicke, Boris T., Redfield, Seth, Dhillon, Vikram S., Marsh, Thomas R., Swan, Andrew
This paper investigates the frequency of transiting planetary systems around metal-polluted white dwarfs using high-cadence photometry from ULTRACAM and ULTRASPEC on the ground, and space-based observations with TESS. Within a sample of 313 metal-pol
Externí odkaz:
http://arxiv.org/abs/2407.21743
Autor:
Aungwerojwit, Amornrat, Gaensicke, Boris T., Dhillon, Vikram S., Drake, Andrew, Inight, Keith, Kaye, Thomas G., Marsh, T. R., Mullen, Ed, Pelisoli, Ingrid, Swan, Andrew
Combining archival photometric observations from multiple large-area surveys spanning the past 17 years, we detect long-term variability in the light curves of ZTFJ032833.52-121945.27 (ZTFJ0328-1219), ZTFJ092311.41+423634.16 (ZTFJ0923+4236) and WD114
Externí odkaz:
http://arxiv.org/abs/2404.04422
Autor:
Pelisoli, Ingrid, Marsh, T. R., Parsons, S. G., Aungwerojwit, A., Ashley, R. P., Breedt, E., Brown, A. J., Dhillon, V. S., Dyer, M. J., Green, M. J., Kerry, P., Littlefair, S. P., Sahman, D. I., Shahbaz, T., Wild, J. F., Chakpor, A., Lakhom, R.
AR Scorpii (AR Sco) is the only radio-pulsing white dwarf known to date. It shows a broad-band spectrum extending from radio to X-rays whose luminosity cannot be explained by thermal emission from the system components alone, and is instead explained
Externí odkaz:
http://arxiv.org/abs/2208.08450
Autor:
Farihi, J., Hermes, J. J., Marsh, T. R., Mustill, A. J., Wyatt, M. C., Guidry, J. A., Wilson, T. G., Redfield, S., Izquierdo, P., Toloza, O., Gänsicke, B. T., Aungwerojwit, A., Dhillon, V. S., Swan, A.
This article reports quasi-continuous transiting events towards WD 1054-226 at d=36.2 pc and V=16.0 mag, based on simultaneous, high-cadence, multi-wavelength imaging photometry using ULTRACAM over 18 nights from 2019 to 2020 March. The predominant p
Externí odkaz:
http://arxiv.org/abs/2109.06183
Autor:
Pelisoli, Ingrid, Marsh, T. R., Ashley, R. P., Hakala, Pasi, Aungwerojwit, A., Burdge, K., Breedt, E., Brown, A. J., Chanthorn, K., Dhillon, V. S., Dyer, M. J., Green, M. J., Kerry, P., Littlefair, S. P., Parsons, S. G., Sahman, D. I., Wild, J. F., Yotthanathong, S.
Accreting magnetic white dwarfs offer an opportunity to understand the interplay between spin-up and spin-down torques in binary systems. Monitoring of the white dwarf spin may reveal whether the white dwarf spin is currently in a state of near-equil
Externí odkaz:
http://arxiv.org/abs/2109.00553
Autor:
Hernandez, M. S., Tovmassian, G., Zharikov, S., Gaensicke, B. T., Steeghs, D., Aungwerojwit, A., Rodriguez-Gil, P.
We analysed a wealth of optical spectroscopic and photometric observations of the bright (V=11.9) cataclysmic variable BG Tri. TheGaiaDR2 parallax gives a distance d=334(8)pc to the source, making the object one of the intrinsically brightest nova-li
Externí odkaz:
http://arxiv.org/abs/2102.00328
Autor:
Chote, P., Gaensicke, B. T., McCormac, J., Aungwerojwit, A., Bayliss, D., Burleigh, M. R., Casewell, S. L., Eigmueller, Ph., Gill, S., Goad, M. R., Hermes, J. J., Jenkins, J. S., Mukadam, A. S., Poshyachinda, S., Raynard, L., Reichart, D. E., Szkody, P., Toloza, O., West, R. G., Wheatley, P. J.
Light curves of the accreting white dwarf pulsator GW Librae spanning a 7.5 month period in 2017 were obtained as part of the Next Generation Transit Survey. This data set comprises 787 hours of photometry from 148 clear nights, allowing the behaviou
Externí odkaz:
http://arxiv.org/abs/2101.08786
Autor:
Hollands, Mark A., Tremblay, Pier-Emmanuel, Gänsicke, Boris T., Camisassa, María E., Koester, Detlev, Aungwerojwit, Amornrat, Chote, Paul, Córsico, Alejandro H., Dhillon, Vik S., Gentile-Fusillo, Nicola P., Hoskin, Matthew J., Izquierdo, Paula, Marsh, Tom R., Steeghs, Danny
White dwarfs are dense, cooling stellar embers consisting mostly of carbon and oxygen, or oxygen and neon (with a few percent carbon) at higher initial stellar masses. These stellar cores are enveloped by a shell of helium which in turn is usually su
Externí odkaz:
http://arxiv.org/abs/2003.00028
Autor:
Pala, A. F., Gänsicke, B. T., Breedt, E., Knigge, C., Hermes, J. J., Fusillo, N. P. Gentile, Hollands, M. A., Naylor, T., Pelisoli, I., Schreiber, M. R., Toonen, S., Aungwerojwit, A., Cukanovaite, E., Dennihy, E., Manser, C. J., Pretorius, M. L., Scaringi, S., Toloza, O.
We present the first volume-limited sample of cataclysmic variables (CVs), selected using the accurate parallaxes provided by the second data release (DR2) of the ESA $\mathit{Gaia}$ space mission. The sample is composed of 42 CVs within $150\,$pc, i
Externí odkaz:
http://arxiv.org/abs/1907.13152
Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0
Autor:
Pala, A. F., Gänsicke, B. T., Marsh, T. R., Breedt, E., Hermes, J. J., Landstreet, J. D., Schreiber, M. R., Townsley, D. M., Wang, L., Aungwerojwit, A., Hambsch, F. -J., Monard, B., Myers, G., Nelson, P., Pickard, R., Poyner, G., Reichart, D. E., Stubbings, R., Godon, P., Szkody, P., De Martino, D., Dhillon, V. S., Knigge, C., Parsons, S. G.
We present high-time-resolution photometry and phase-resolved spectroscopy of the short-period ($P_\mathrm{orb} = 80.52\,\mathrm{min}$) cataclysmic variable SDSS J123813.73-033933.0, observed with the $\mathit{Hubble}$ $\mathit{Space}$ $\mathit{Teles
Externí odkaz:
http://arxiv.org/abs/1811.05981