Bolometric light curve and ejecta mass
Bolometric corrections for optical light curves of core-collapse supernovae
... evolve strongly with respect to time, as has been indicated previ- ously for individual or small samples of events (e.g. Valenti et al. 2008; Modjaz et al. 2009; Stritzinger et al. 2009). This behaviour appears to be ...
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ON THE PERIOD AND LIGHT CURVE OF THE
... 2010). Binnendijk (pp. 218-221) defined two varieties of these W UMa systems, A-types, with transit primary eclipses, and W-types, with occultation primaries. Given the direct dependence of the ratio of radii on ...
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Multiwavelength light curve parameters of Cepheid variables
... observed light curves of Cepheid variables using Fourier ...theoretical light curves at multi- ple wavelengths are generated using stellar pulsation models for chemical compositions representative of ...
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Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
... halo mass, we compare the AGN model (blue curve), which includes AGN feedback, to the REF ...stellar ejecta are deposited, we again expect a low recycling-fuelled SFR if the AGN feedback is strong ...
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VBbinarylensing : a public package for microlensing light curve computation
... Finally, an important information for the user is the parameter range in which the code is robust and can be used safely. We have already declared the ranges spanned in the detailed maps used for the definition of our ...
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The Double-peaked Radio Light Curve of Supernova PTF11qcj
... radio light curve shows a double–peak profile, possibly associated with density variations in the circumstellar medium (CSM), or with the presence of an off-axis GRB ...radio light curve do ...
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A Hubble Space Telescope transit light curve for GJ 436b
... This value and our measured transit times will serve as important benchmarks in future studies of the GJ 436 system. Key words. techniques: photometric – eclipses – stars: individual: GJ 436 – stars: planetary systems 1. ...
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NEW LIGHT-TIME CURVE OF ECLIPSING BINARY AM Leo
... Albayrak et al. (2005a) obtained the mutual orbital period of AM Leo and the third body by the very eccentric orbit to be about 45 years, they also estimated the mass of the third body to be M 3 = 0.18M ⊙ . These ...
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The Light Curve and the Orbital Period Variations of Binary System TT Andromedae
... photoelectric light curve analysis of the TT And system in a broad band filter (400 - 700 nm) was carried out using the PHOEBE ...low mass of the cooler component ...
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SAMBA: SUPERCONDUCTING ANTENNA-COUPLED, MULTI-FREQUENCY, BOLOMETRIC ARRAY
... Multi-frequency, Bolometric Array archi- tecture promises a lot of advantages compared to existing ...stray light and out-of-band ...plane mass and volume would be eliminated by the new focal plane ...
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FIRST SOLUTION OF THE LIGHT CURVE OF THE NEW VARIABLE STAR 3UC 281-203711
... Nothing was known about the physical nature of components of this eclipsing binary system. Hence, the initial values of physical parameters were chosen on the basis of values of the period, surface brightness ratio, ...
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Light Curve Plotting with AstroImageJ & Excel
... When you have carried out your measurements and obtained your data, you will present your results on graphs to display the light curves of the target. Prior to carrying out this activity, if you have not used the ...
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Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities
... total mass of M ∼ ...total mass of the remnant is below the maximum allowed mass of a spheri- cally symmetric star for the given ...maximum mass of ∼ ...
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Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
... global mass-loss history of each galaxy from an empirically motivated distribution of stellar population ages and a set of stellar yields and lifetimes, and showed that the gas from stellar mass-loss can ...
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Ejecta Cone Angle and Ejecta Size Following a Non-perforating Hypervelocity Impact
... Keywords: Ejecta length; Ejecta ring; Scalling law; No perforation; Cratering ...These ejecta and fragments have the potential to become space debris (known as secondary ...
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An Observational Determination of the Bolometric Quasar Luminosity Function
... single bolometric QLF self-consistently reproduces the observed QLFs in all bands and at all redshifts for which we compile ...self-consistent bolometric QLF and there is no evidence for any additional ...
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An Observational Determination of the Bolometric Quasar Luminosity Function
... single bolometric QLF self-consistently reproduces the observed QLFs in all bands and at all redshifts for which we compile ...self-consistent bolometric QLF and there is no evidence for any additional ...
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Investigation of bolometric and resistive properties of nickel oxide
... 97 Chapter 5 Conclusions Nickel was successfully oxidized through a furnace thermal oxidation process, involving a 500 °C soak in dry O 2 for 5 hours. Through various means of characterization, the bolometric and ...
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Machine Learning Techniques for Stellar Light Curve Classification
... Kepler light curves from the Mikulski Archive for Space Telescopes ( MAST ) to classify according to 10 distinct physical properties using both representation learning and feature engineering ...real ...
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Evaluating elliptic curve based KEMs in the light of pairings
... elliptic curve KEMs proposed to be standardized when they are implemented on pairing ...random curve results in a secure ...random curve, the elliptic curve KEMs present a very tight security ...
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