The HU Aqr planetary system hypothesis revisited
@article{Godziewski2014TheHA, title={The HU Aqr planetary system hypothesis revisited}, author={Krzysztof Goździewski and Aga Słowikowska and Dinko P. Dimitrov and Krzysztof Krzeszowski and Michal Zejmo and G.Kanbach and Vadim Burwitz and Arne Rau and P. Irawati and Andrea Richichi and Marcin P. Gawroński and Grzegorz Nowak and Ilham Nasiroglu and Dominik J{\'o}zef Kubicki}, journal={Monthly Notices of the Royal Astronomical Society}, year={2014}, volume={448}, pages={1118-1136} }
We study the mid-egress eclipse timing data gathered for the cataclysmic binary HU Aquarii during the years 1993-2014. The (O-C) residuals were previously attributed to a single ~7 Jupiter mass companion in ~5 au orbit or to a stable 2-planet system with an unconstrained outermost orbit. We present 22 new observations gathered between June, 2011 and July, 2014 with four instruments around the world. They reveal a systematic deviation of ~60 - 120 seconds from the older ephemeris. We re-analyse…
Figures and Tables from this paper
24 Citations
Is There a Circumbinary Planet around NSVS 14256825?
- Physics, Geology
- 2017
The cyclic behavior of (O–C) residuals of eclipse timings in the sdB+M eclipsing binary NSVS 14256825 was previously attributed to one or two Jovian-type circumbinary planets. We report 83 new…
High-speed photometry of the eclipsing polar UZ Fornacis
- Physics, GeologyAstronomy & Astrophysics
- 2019
We present 33 new mid-eclipse times spanning approximately eight years of the eclipsing polar UZ Fornacis. We have used our new observations to test the two-planet model previously proposed to…
The conjectured S-type retrograde planet in ν Octantis: more evidence including four years of iodine-cell radial velocities
- Geology, Physics
- 2016
We report 1212 radial-velocity (RV) measurements obtained in the years 2009–2013 using an iodine cell for the spectroscopic binary ν Octantis (K1 III/IV). This system (abin ∼ 2.6 au, P ∼ 1050 d) is…
New observations of the eclipsing binary system NY Vir and its candidate circumbinary planets
- Physics, GeologyMonthly Notices of the Royal Astronomical Society
- 2021
As a result of various studies, it has been determined that several post-common envelope eclipsing binaries have variations in their orbital periods. These variations are thought to be caused by…
Eclipsing time variations in close binary systems: Planetary hypothesis vs. Applegate mechanism
- Physics
- 2015
The observed eclipsing time variations in post-common-envelope binaries (PCEBs) can be interpreted as potential evidence for massive Jupiter-like planets, or as a result of magnetic activity, leading…
DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet
- Physics, GeologyThe Astrophysical Journal
- 2018
We present a timing analysis of the eclipsing post-common envelope binary (PCEB) DE CVn. Based on new CCD photometric observations and published data, we found that the orbital period in DE CVn has a…
Solar System Physics for Exoplanet Research
- Geology, PhysicsPublications of the Astronomical Society of the Pacific
- 2020
Over the past three decades, we have witnessed one of the great revolutions in our understanding of the cosmos—the dawn of the Exoplanet Era. Where once we knew of just one planetary system (the…
Z Draconis with two companions in a 2:1 mean-motion resonance
- Physics
- 2014
All available mid-eclipse times of the eclipsing binary Z Draconis are analyzed, and three sets of cyclic variations with periods of 20.1, 29.96 and 59.88 yr are found. The low-amplitude variations…
A close-in substellar object orbiting the sdOB-type eclipsing-binary system NSVS 14256825
- Physics, GeologyResearch in Astronomy and Astrophysics
- 2019
NSVS 14256825 is the second discovered sdOB+dMeclipsing-binary system with an orbital period of 2.65 h. This special binary was reported to contain circumbinary planets or brown dwarfs by using the…
Cyclic Period Oscillation of the Eclipsing Dwarf Nova DV UMa
- Physics
- 2017
DV UMa is an eclipsing dwarf nova with an orbital period of ∼2.06 hr, which lies just at the bottom edge of the period gap. To detect its orbital period changes, we present 12 new mid-eclipse times…
References
SHOWING 1-10 OF 75 REFERENCES
Revisiting the proposed planetary system orbiting the eclipsing polar HU Aquarii
- Physics, Geology
- 2011
It has recently been proposed, on the basis of eclipse-timing data, that the eclipsing polar cataclysmic variable HU Aquarii is host to at least two giant planets. However, that result has been…
A dynamical analysis of the proposed HU Aquarii planetary system
- Physics, Geology
- 2011
It has recently been suggested that the eclipsing polar HU Aquarii is a host to at least two giant planets. We have performed highly detailed dynamical analyses of the orbits of those planets and…
On the HU Aquarii planetary system hypothesis
- Physics, Geology
- 2012
In this paper, we investigate the eclipse timing of the polar binary HU Aquarii that has been observed for almost two decades. Recently, Qian et al. attributed large (O–C) deviations between the…
Testing the planetary models of HU Aquarii
- Physics, Geology
- 2014
We present new eclipse observations of the polar (i.e. semidetached magnetic white dwarf + M-dwarf binary) HU Aqr, and mid-egress times for each eclipse, which continue to be observed increasingly…
On the ephemeris of the eclipsing polar HU Aquarii
- Physics, Geology
- 2014
The magnetic cataclysmic variable HU Aquarii displayed pronounced quasi-periodic modulations of its eclipse timing. These were interpreted in terms of the light-travel time (LTT) effect caused by a…
Detection of a planetary system orbiting the eclipsing polar HU Aqr
- Physics, Geology
- 2011
Using the precise times of mid-egress of the eclipsing polar HU Aqr, we discovered that this polar is orbited by two or more giant planets. The two planets detected so far have masses of at least 5.9…
A dynamical analysis of the proposed circumbinary HW Virginis planetary system
- Physics, Geology
- 2012
In 2009, the discovery of two planets orbiting the evolved binary star system HWVirginis (HWVir) was announced, based on systematic variations in the timing of eclipses between the two stars. The…
The quest for companions to post-common envelope binaries - III. A reexamination of HW Virginis
- Physics, Geology
- 2012
We report new mid-eclipse times of the short-period sdB/dM binary HW Virginis, which differ substantially from the times predicted by a previous model. The proposed orbits of the two planets in that…
Testing a hypothesis of the ν Octantis planetary system
- Physics
- 2013
We investigate the orbital stability of a putative Jovian planet in a compact binary \nu Octantis reported by Ramm et al. We re-analyzed published radial velocity data in terms of self-consistent…
TWO POSSIBLE CIRCUMBINARY PLANETS IN THE ECLIPSING POST-COMMON ENVELOPE SYSTEM NSVS 14256825
- Physics, Geology
- 2013
We present an analysis of eclipse timings of the post-common envelope binary NSVS 14256825, which is composed of an sdOB star and a dM star in a close orbit (Porb = 0.110374 days). High-speed…