Results 1 to 10 of about 200,082 (276)

Mass Ejection from the Symbiotic Prototype Z and During its 2006 Outburst

open access: yesOpen Astronomy, 2012
High-resolution spectroscopic observations in the region of the Balmer Hα and Hγ lines of the symbiotic binary Z And were performed during its major eruption in 2006.
Tomov N. A.   +2 more
doaj   +1 more source

Symbiotic Nova PU Vul - 33 Years of Observations

open access: yesOpen Astronomy, 2012
We present UBVRI light curves of the symbiotic nova PU Vul after its outburst in 1978. Three observed eclipses of the hot component by the cool one were used to determine the ephemeris of the binary system as JD (Min I) = 2444550(15) + 4897(10) × E days.
Shugarov S., Chochol D., Kolotilov E.
doaj   +1 more source

Deconstructing the Characteristics of the Ionized Gas Component in Planetary Nebulae From Their Internal Motions

open access: yesFrontiers in Astronomy and Space Sciences, 2022
The internal motions of the ionized gas in the shells of planetary nebulae (PNe) have served as relevant diagnostic tools to understand the development of this important stage of stellar evolution.
J. A. López
doaj   +1 more source

Photometric Activity of the Symbiotic Star CH Cyg During 2008–2011

open access: yesOpen Astronomy, 2012
We present results of UBVRC observations of the symbiotic star CH Cyg before and after optical and X-ray bursts in 2009 at various timescales. Rapid variability was found only during a strong burst (U ~ 9.5 mag) in 2009 October, while during the low ...
Shugarov S.   +4 more
doaj   +1 more source

Are sdAs helium core stars?

open access: yesOpen Astronomy, 2017
Evolved stars with a helium core can be formed by non-conservative mass exchange interaction with a companion or by strong mass loss. Their masses are smaller than 0.5 M⊙. In the database of the Sloan Digital Sky Survey (SDSS), there are several thousand
Pelisoli Ingrid   +2 more
doaj   +1 more source

Evaluating GAIA performances on eclipsing binaries. I. Orbits and stellar parameters for V505 Per, V570 Per and OO Peg [PDF]

open access: yes, 2001
The orbits and physical parameters of three detached, double-lined A-F eclipsing binaries have been derived combining H_P, V_T, B_T photometry from the Hipparcos/Tycho mission with 8500-8750 Ang ground-based spectroscopy, mimicking the photometric ...
A. Prša   +26 more
core   +4 more sources

Beyond binaries and before becoming: Reconsidering resistance in UK higher education

open access: yesPRISM, 2023
Drawing from the tensions within non-representational and human practice perspectives on affect, this paper continues the task of re-conceptualising academic-level resistance in the context of UK higher education. Such re-conceptualisation is underpinned
Mollie Baker
doaj   +1 more source

Dynamics of black holes in de Sitter spacetimes [PDF]

open access: yes, 2012
Nonlinear dynamics in cosmological backgrounds has the potential to teach us immensely about our Universe, and also to serve as prototype for nonlinear processes in generic curved spacetimes.
Cardoso, Vitor   +5 more
core   +2 more sources

The evolution of photo-evaporating viscous discs in binaries [PDF]

open access: yes, 2017
A large fraction of stars are in binary systems, yet the evolution of proto-planetary discs in binaries has been little explored from the theoretical side.
Clarke, Cathie J., Rosotti, Giovanni P.
core   +2 more sources

The BSN Application-I: Photometric Light Curve Solutions of Contact Binary Systems

open access: yesGalaxies
Light curve analysis of W UMa-type contact binary systems using MCMC or MC methods can be time-consuming, primarily because the repeated generation of synthetic light curves tends to be relatively slow during the fitting process.
Ehsan Paki   +2 more
doaj   +1 more source

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