Rice D., Steffen J. H., Vazan A. (2024): “The Distribution of Planet Radius in Kepler Multiplanet System Depends on Gap Complexity” – The Astrophysical Journal Letters, Volume 973, Issue 1, id.L4, 9pp.
Vazan A., Ormel C.W., Brouwers M. G. (2024): “How planets grow by pebble accretion V: Silicate rainout delays contraction of sub-Neptunes” –Astronomy & Astrophysics, Volume 687, id.A262, 14 pp.
Barat S., Desert JM.,
Vazan A., et al. (2024): “The metal-poor atmosphere of a potential sub-Neptune progenitor” –
Nature Astronomy, advanced online submission, 86B
Vazan A. & Ormel C.W. (2023): “Rocky sub-Neptunes formed by pebble accretion: Rain of rocks from polluted envelopes” - Asstronomy & Astrophysics, Volume 676, id.L8, 7 pp.
Podolak M., Levi A., Vazan A., Malamud U. (2023): “An equation of state of CO for use in planetary modeling” - Icarus, Volume 394, article id. 115424.
Pan S., Huang T., Vazan A., et al. (2023): “Magnesium oxide-water compounds at megabar pressure and implications on planetary interiors” - Nature Communications, Volume 14, article id. 1165.
Miguel Y. & Vazan A. (2023) : “Interior and Evolution of the Giant Planets” - Remote Sensing, vol. 15, issue 3, p. 681.
Vazan A., Sari R., Kessel R. (2022) “A new perspective on interiors of ice-rich planets: Ice-rock mixture rather than ice on top of rock" - The Astrophysical Journal, Volume 926, Issue 2, id.150, 12 pp
Ormel
C., Vazan A., Brouwers M. (2021) “How planets grow by pebble
accretion. III. Emergence of an interior composition gradient” - Astronomy
& Astrophysics, Volume 647, id.A175, 19
Vazan A. & Helled R. (2020). “Explaining the low luminosity of Uranus: A self-consistent thermal and structural evolution” - Astronomy & Astrophysics, Volume 633, id.A50, 10 pp.
Vazan A. & Sari R. (2020). ”On the aspect ratio of ’Oumuamua :regular shape and irregular surface” - Monthly Notices of the Royal Astronomical Society, Volume 493, Issue 2, p.1546-1552.
Humphries J., Vazan A., Bonavita M., Helled R., Nayakshin S. (2019). “Constraining the initial planetary population in the gravitational instability model” - Monthly Notices of the Royal Astronomical Society, Volume 488, Issue 4, p.4873-4889.
Vazan A., Ormel C. W., Noack L., Dominik C. (2018) “Contribution of the core to the thermal evolution of sub-Neptunes” - The Astrophysical Journal, Volume 869, Issue 2, article id. 163, 11 pp.
Vazan A., Helled R., Guillot T. (2018). “Jupiter's evolution with primordial composition gradients” - Astronomy & Astrophysics Letters, Volume 610, L14.
Vazan A., Ormel C. W., Dominik C. (2018). “Effect of core cooling on the radius of sub-Neptune planets” - Astronomy & Astrophysics Letters, Volume 610, id.L1, 4 pp.
Brouwers M. G., Vazan A., Ormel C. W. (2018). “How cores grow by Pebble Accretion” - Astronomy & Astrophysics, Volume 611, id.A65, 12 pp.
Vazan A., Helled R., Podolak M., Kovetz A. (2016). "The evolution and internal structure of Jupiter and Saturn with compositional gradients” - The Astrophysical Journal, Volume 829, Issue 2, article id. 118, 11 pp.
Vazan A., Helled R., Kovetz A., Podolak M. (2015). "Convection and mixing in giant planet evolution” - The Astrophysical Journal, Volume 803, Issue 1, article id. 32, 11 pp.
Vazan A., Kovetz A., Podolak M., Helled R. (2013). "The effect of composition on the evolution of giant and intermediate-Mass Planets" - Monthly Notices of the Royal Astronomical Society, Volume 434, Issue 4, p.3283-3292.
Vazan A. & Helled R. (2012). "On the evolution and survival of protoplanets embedded in a protoplanetary disk” - The Astrophysical Journal, Volume 756, Issue 1, article id. 90, 11 pp.