Results 131 to 140 of about 85,351 (144)
Some of the next articles are maybe not open access.
The nova type outburst of the symbiotic star AS 296
International Astronomical Union Colloquium, 1990AbstractThe photometric and spectroscopic evolutions, displayed by AS 296 since the June 1988 outburst ([1]), are presented and discussed. The main features of the model outlined by [2], [3] and [4], are confirmed and further developped. An orbital period of about 3 years is inferred from Hα modulation (see [5]).The outburst originated from a TNR event
openaire +1 more source
The Slow Nova RR Tel and the Symbiotic Stars
1977The slow nova RR Tel belongs to a group of symbiotic stars which contain in addition to an M type component, a hot dust shell. For symbiotics without dust, infrared photometry shows that the M component is constant in light. For these systems the mass exchange is usually considered to be through the inner Lagrangian point.
openaire +1 more source
Photoionization Modelling of Quiescence-Phase Spectra of Novae and a Symbiotic Star
Monthly Notices of the Royal Astronomical Society, 2020Ramkrishna Das +2 more
exaly
Recurrent and Symbiotic Novae in Data From the Optical Gravitational Lensing Experiment
Monthly Notices of the Royal Astronomical Society, 2014Przemek Mroz +2 more
exaly
On the Late-Type Components of Slow Novae and Symbiotic Stars
Monthly Notices of the Royal Astronomical Society, 1980David A Allen
exaly
On the new minimum of the symbiotic nova PU Vulpeculae
Monthly Notices of the Royal Astronomical Society, 1995E. A. Kolotilov, U. Munari, B. F. Yudin
openaire +1 more source

