TACOS: <i>TESS</i> AM CVn Outbursts Survey
نویسندگان
چکیده
ABSTRACT Using Transiting Exoplanet Survey Satellite (TESS), we are doing a systematic study of outbursting AM CVn systems to place some limits on the current outbursts models. We present TESS light curve (LC) for 9 CVns showing both superoutbursts (SOs) and normal (NOs). The continuous coverage with allows us stringent duration structures SOs NOs. evidence that in at least enhanced mass transfer (EMT) has be taken into account explain observed LC rebrighthening phase after SOs. For others, colour evolution from simultaneous observations g r ZTF differs previously reported longer period where EMT is responsible SO. also find due lack sufficiently high cadence many might have been overestimated previous ground-based surveys. report SO 6 CVns. found precursors common feature seen 5 Finally, 10-min 2-min LCs allowed two new candidate orbital periods CVns, which reasonably good agreement predictions their based past outburst histories.
منابع مشابه
AM CVn stars
I review our observational and theoretical knowledge of AM CVn stars, focusing on recent developments. These include newly discovered systems, the possibility that two recently discovered extremely short period objects are AM CVn stars and an update on X-ray, UV an optical studies. Theoretical advances include the study of the details of both the donor and accretor, and the physics of the heliu...
متن کاملAm Cvn Stars in the Uct Ccd Cv Survey
High speed photometry of the helium-transferring binary ES Cet – taken over a two-year period (2001 October – 2003 October) – shows a very stable photometric period of 620.211437 ± 0.000038 s, with a tentative indication of curvature in the O–C diagram suggesting a change in period at a rate of Ṗ ∼ 1.6×10 . Phase-resolved spectroscopy of ES Cet obtained with the Hobby-Eberly Telescope shows a c...
متن کاملThe new AM CVn star in Hydra
High speed photometry of the new AM CVn star in Hya (previously known as SN2003aw), spectroscopically identified by Chornock & Filippenko, shows it to have a superhump period of 2041.5 ± 0.3 s. We find a range of brightness from V ∼ 16.5 to 20.3, presumably caused by variations in the rate of mass transfer. In the intermediate state the system cycles in brightness with a period of ∼ 16 h and ra...
متن کاملThe AM CVn binary SDSSJ173047.59+554518.5
The AM Canum Venaticorum (AM CVn) binaries are a rare group of hydrogendeficient, ultra-short period, mass-transferring white dwarf binaries, and are possible progenitors of type Ia supernovae. We present time-resolved spectroscopy of the recently-discovered AM CVn binary SDSS J173047.59+554518.5. The average spectrum shows strong double-peaked helium emission lines, as well as a variety of met...
متن کاملThe outburst properties of AM CVn stars
We briefly summarize the observational properties of ultra-compact binaries called AM CVn stars. We analize their outbursts originating from the thermal-viscous instability in helium accretion disc. We present our preliminary results in applying the model of Dwarf Novae outbursts to helium discs. We can calculate models of outbursts of reasonable amplitude of 2 mag with a constant α parameter t...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2021
ISSN: ['0035-8711', '1365-8711', '1365-2966']
DOI: https://doi.org/10.1093/mnras/stab2685