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Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 01/2020, Volume 491, Issue 1, pp. L34 - L39
ABSTRACT During the runaway phase of their formation, gas giants fill their gravitational spheres of influence out to Bondi or Hill radii. When runaway ends,... 
Physics - Earth and Planetary Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 464, Issue 4, pp. 3937 - 3937
Short-period Earth to Neptune-sized exoplanets (super-Earths) with voluminous gas envelopes seem to be very common. These gas atmospheres are thought to have... 
Planetary atmospheres | Planets | Atmospheres | Heating | Tidal effects | Extrasolar planets | Stars | Nebulae
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 464, Issue 4, p. 3937
  Short-period Earth to Neptune-sized exoplanets (super-Earths) with voluminous gas envelopes seem to be very common. These gas atmospheres are thought to have... 
Earth | Gases | Heating | Atmosphere | Tides | Astronomy
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 07/2019, Volume 487, Issue 1, pp. 681 - 690
Gas giants are thought to form by runaway accretion: an instability driven by the self-gravity of growing atmospheres that causes accretion rates to rise... 
PLANETS | CORE | planets and satellites: gaseous planets | T TAURI STARS | PROTOPLANETS | VISCOSITY | ACCRETION DISKS | planet-disc interactions | DISTRIBUTIONS | MODELS | ASTRONOMY & ASTROPHYSICS | SOLAR | ROSSBY-WAVE INSTABILITY | planets and satellites: formation | Physics - Earth and Planetary Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 12/2019, Volume 490, Issue 3, pp. 4334 - 4343
Giant planets are thought to form by runaway gas accretion on to solid cores. Growth must eventually stop running away, ostensibly because planets open gaps... 
PLANETS | INITIAL CONDITIONS | CORE ACCRETION | planets and satellites: gaseous planets | INSTABILITY | GASEOUS ENVELOPE | FINAL MASSES | PROTOPLANETS | ATMOSPHERES | MODELS | DISKS | ASTRONOMY & ASTROPHYSICS | planets and satellites: formation | Physics - Earth and Planetary Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2016, Volume 825, Issue 1, pp. 29 - 29
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2018, Volume 476, Issue 1, pp. 759 - 765
Recent observations identify a valley in the radius distribution of small exoplanets, with planets in the range 1.5-2.0 R. significantly less common than... 
Planets and satellites: Atmospheres | Planets and satellites: Physical evolution | PLANETS | planets and satellites: physical evolution | planets and satellites: atmospheres | STARS | SUPER-EARTHS | ASTRONOMY & ASTROPHYSICS | Physics - Earth and Planetary Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2018, Volume 479, Issue 2, pp. 1986 - 1996
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/2014, Volume 780, Issue 1, pp. 18 - 12
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2016, Volume 819, Issue 2, p. 116
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 464, Issue 4, pp. 3937 - 3944
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2015, Volume 803, Issue 2, pp. 111 - 9
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 07/2017, Volume 469, Issue 1, pp. 278 - 285
The orbits of many observed hot Jupiters are decaying rapidly due to tidal interaction, eventually reaching the Roche limit. We analytically study the ensuing... 
planets and satellites: gaseous planets | IN-SITU FORMATION | INSTABILITY | SUPER-EARTHS | planets and satellites: composition | planet-star interactions | SOLID CORES | TIDAL DISSIPATION | EVOLUTION | GIANT PLANET FORMATION | ASTRONOMY & ASTROPHYSICS | GAS | ACCRETION | SOLAR-TYPE STARS | Physics - Earth and Planetary Astrophysics
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 2016, Volume 822, Issue 1, pp. L11 - L11
Journal Article
01/2020
Black widows are close binary systems in which a millisecond pulsar is orbited by a companion a few per cent the mass of the sun. It has been suggested that... 
Physics - High Energy Astrophysical Phenomena
Journal Article
08/2018
We present visible-light and ultraviolet (UV) observations of the supernova PTF12glz. The SN was discovered and monitored in near-UV and R bands as part of a... 
Journal Article
by Eizenberg, H and Tanaami, Z and Jacobsohn, R and Lalazar, A and Hayut, M and Sibony, M and Sibony, M and Sibony, M and Tal, A and Rubin, B and Yossef, T and Plakhine, D and Plakhine, D and Kleifeld, Y and Kleifeld, Y and Weinberg, T and Lior, E and Avdat, N and Portnoy, V H and Katzir, N and Joel, D M and Buxbaum, H and Goldwasser, Y and Hershenhorn, J and Hershenhorn, J and Zamski, E and Kleifeld, Y and Goldwasser, Y and Hershenhorn, Y and Golan, S and Herzlinger, G and Chilf, T and Losner-Goshen, Dalia and Portnoy, V H and Joel, D M and Aly, R and Halpern, N and Blumenfeld, T and Shomer-Ilan, Adiva and Mayer, A M and Bar-Nun, Nurit and Ben-Hod, G and Amsellem, Ziva and Gressel, J and Gressel, J and Kernyi, Z and Hornok, L and Cohen, B and Amsellem, Ziva and Sharon, A and Sharon, A and Kitahin, S and Bosak, A and Bosak, A and Bar-Peled, Y and Barnea, N and Yasour, H and Hayut, M and Tal, A and Alon, Y and El-Nahhal, Y Z and Nir, S and Polubesova, T and Margulies, L and Siti, E and Kaplan, Ch and Levanon, I and Gokkes, M and Gokkes, M and Hadar, A and Chachlon, Y and Yovel, H and Colodney, G and Glidai, S and Tal, Shuli and Nir, A and Yasur, E and Kigel, J and Kigel, J and Yaacoby, T and Nir, A and Ye, Bin and Gressel, J and Kimel, U and Manulis, Shulamit and Kleitman, Frida and Dror, Orit and Chalupowicz, Laura and Khayat, E and Tsror (Lahkim), Leah and Erlich, Orly and Menashe, A and Wysoki, M and Gerson, U and Slabezki, Y and Dag, A and Efrat, H and Yacobson, B and Palevsky, E and Reuveny, H and ...
Phytoparasitica, ISSN 0334-2123, 6/1999, Volume 27, Issue 2, pp. 109 - 168
Journal Article