A. Kovetz

Tel Aviv University — Israel

Physics and Astronomy · Physical Sciences

23h-index2.4kcitations133works0.02yr avg
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Research Topics

Stellar, planetary, and galactic studies(46), Astrophysical Phenomena and Observations(30), Astro and Planetary Science(25), Astronomy and Astrophysical Research(24), Gamma-ray bursts and supernovae(23)

Publications133 total

A unified theory of cataclysmic variable evolution from feedback-dominated numerical simulations
Nature Astronomy·2020· 54 cited
A unified theory of cataclysmic variables from self-consistent numerical simulations
arXiv (Cornell University)·2020Open Access
Multi-outburst nova modeling & where models meet observations
Advances in Space Research·2019· 9 cited
Modeling the evolution of ice-rich planets
AAS/Division for Extreme Solar Systems Abstracts·2019
At the forefront of multi-outburst modeling of nova explosions
42nd COSPAR Scientific Assembly·2018
A Hubble Space Telescope survey for novae in M87 – III. Are novae good standard candles 15 d after maximum brightness?
Monthly Notices of the Royal Astronomical Society·2017· 5 citedOpen Access
An Extensive Grid of Models Producing Extreme Horizontal Branch Stars
arXiv (Cornell University)·2017· 2 citedOpen Access
A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae<sup>*</sup>
The Astrophysical Journal·2017· 32 citedOpen Access
Novae are good standard candles at 15 days after maximum light
arXiv (Cornell University)·2017· 1 citedOpen Access
A Hubble Space Telescope Survey for Novae in M87. III. Novae as Effective Standard Candles
arXiv (Cornell University)·2017Open Access
Alternative Evolution and Internal Structure for Jupiter and Saturn
2016
Alternative Evolution and Internal Structure for Jupiter and Saturn
DPS·2016
Long Term Modelling of Recurrent Novae Resulting in SNIa
2015
WDs in Binaries That Can Lead to SNIa
EAS Publications Series·2015
Features of Nova Outburst Light Curves as Derived from Modeling
2014
Observational signatures of SNIa progenitors, as predicted by models
Monthly Notices of the Royal Astronomical Society·2014· 51 citedOpen Access
Composition Effect on Mass-Radius Relation of Exoplanets
EGU General Assembly Conference Abstracts·2014
Giant Planet Evolution: The Effect of Convection and Mixing
EPSC·2014
Nova multiwavelength light curves: predicting UV precursor flashes and pre-maximum halts
Monthly Notices of the Royal Astronomical Society·2013· 47 citedOpen Access
The effect of composition on the evolution of giant and intermediate-mass planets
Monthly Notices of the Royal Astronomical Society·2013· 117 citedOpen Access
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Frequent Co-authors

Dina Prialnik(20), Michael M. Shara(9), G. Shaviv(8), M. Podolak(5), Ravit Helled(5), O. Yaron(5), Yael Hillman(4), James D. Neill(3), David Zurek(3), Allona Vazan(2), Trisha F. Doyle(2), Tod R. Lauer(2), Edward A. Baltz(2), Juan P. Madrid(2), J. Mikołajewska(2), D. L. Welch(2), M. Enosh(2), Amos Harpaz(2), B. Olund(1), Mario Livio(1)