Hot Jupiters
Evaporation of hot jupiters and hot neptunes
... Abstract. Among the nearly five hundred extra-solar planets known, almost 30% orbit closer than 0.1 AU from their parent star. We will review the observa- tions and the corresponding models of the evaporation of these ...
6
New transiting hot Jupiters discovered by WASP South, Euler/CORALIE, and TRAPPIST South
... The figure illustrates that the new systems lie within known pa- rameter space, while being well distributed within the space. As is well established, the more massive planets are less likely to be highly bloated (top ...
13
Exploring Exoplanets' Spectroscopic Secrets: Clues on the Migration and Formation of Hot Jupiters
... rotating hot Jupiters, near-infrared emission from the dayside is likely to be most readily ...the hot gas giants HD 88133 b (Chapter 4), ups And b (Chapter 5), and KELT-2Ab (Chapter ...
150
HATS-25b through HATS-30b: a half-dozen new inflated transiting hot jupiters from the HATSouth survey
... In this work we report the discovery of six new, well – characterized transiting hot Jupiters using the HATSouth global network of automated telescopes ( Bakos et al. 2013 ) , all of which are in fl ated ...
18
Chemical and dynamical processes in the atmospheres of I Ancient and present day earth; II Jupiter and Galilean satellites; III Extrasolar "hot Jupiters"
... oxidants produced on the surface can be delivered to the liquid ocean, if one exists, underneath the surface and thus provide the required energy for underlying ecosystem. The last two chapters are for the exploration of ...
238
WASP 113b and WASP 114b, two inflated hot Jupiters with contrasting densities
... WASP-113 is at the end of its main sequence life. We esti- mate that owing the expansion of the star after the end of the main sequence the planet will be engulfed in ∼1.4 Gyr. The re- sponse of the planetary radius to ...
9
Three irradiated and bloated hot Jupiters: WASP 76b, WASP 82b, and WASP 90b
... transiting hot Jupiters have been found by WASP and the similar ground-based survey HATnet (Bakos et ...radius Jupiters could simply be a selection ...
7
HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey
... so-called hot Jupiters, ...since hot Jupiters are more massive and larger than rocky planets, it is possible to measure their physical parameters with much better accuracy: in primis mass and ...
13
Magnetic activity and hot Jupiters of young Suns : the weak line T Tauri stars V819 Tau and V830 Tau
... of hot Jupiters (hJs) at an early stage in the life of low-mass stars and their planets, and thus for verifying whether core accretion coupled to migration is indeed the best option for forming close-in ...
14
Discovery of three new transiting hot Jupiters: WASP 161 b, WASP 163 b and WASP 170 b
... We present the new discovery of three new transiting hot-Jupiters by the WASP-South project, WASP-161 b, WASP-163 b and WASP-170 b. Follow-up radial velocities obtained with the Euler/CORALIE spectrograph ...
14
WASP South hot Jupiters : WASP 178b, WASP 184b, WASP 185b & WASP 192b
... of hot Jupiters and bloated radii is now well established ...hottest hot Jupiters to be more massive than ...transiting hot Jupiter is ∼ ...
9
HATS-31b through HATS-35b: five transiting hot Jupiters discovered by the HATSouth survey
... transiting hot Jupiters with well determined masses and radii discovered to date retrieved from the NASA Exoplanet Archive 16 on 2016 May 30, with HATS-31b through HATS- 35b superimposed in ...
16
The EBLM Project : IV Spectroscopic orbits of over 100 eclipsing M dwarfs masquerading as transiting hot Jupiters
... 2014; Hatzes & Rauer 2015; Chen & Kipping 2016). To further the comparison, gas giants, brown dwarfs and very low-mass stars also have have similar temperatures in addition to simi- lar sizes. ...
38
Spin-orbit alignment for three transiting hot Jupiters: WASP-103b, WASP-87b, and WASP-66b
... high-obliquity hot Jupiters are indeed the result of primordial disk misalignments, then there should be a signi fi cant number of debris disks observed to be in misalignment with the spin axis of their host ...
16
Stellar obliquities and planetary alignments (SOPA). I. Spin-orbit measurements of three transiting hot Jupiters: WASP-72b, WASP-100b, and WASP-109b
... SuperWASP, Pollacco et al. 2006; HAT, Bakos et al. 2004; KELT, Pepper et al. 2007; CSTAR, Wang et al. 2014 ) , which constitute the major fraction ( about two-thirds ) of all currently known hot Jupiters, ...
12
Two new HATNet hot Jupiters around A stars, and the first glimpse at the occurrence rate of hot Jupiters from TESS*
... of hot Jupiters around evolved stars. These studies suggest that hot Jupiters undergo tidal orbital decay when a star begins evolving into a sub- giant (Schlaufman & Winn ...numerous ...
32
WASP 169, WASP 171, WASP 175 and WASP 182 : three hot Jupiters and one bloated sub Saturn mass planet discovered by WASP south
... three hot Jupiters and one bloated sub-Saturn mass planet: WASP-169b, WASP-171b, WASP-175b, and WASP-182b, all orbiting relatively bright G- and F-type ...
10
Kepler constraints on planets near hot Jupiters
... in hot Jupiter systems— none in nearby orbits ...to hot Jupiters (26). Hot Jupiters are, however, known to have dis- tant stellar or planetary companions (27, ...that hot ...
6
Magnetic activity and hot Jupiters of young Suns: the weak line T Tauri stars V819 Tau and V830 Tau
... of hot Jupiters (hJs) at an early stage in the life of low-mass stars and their planets, and thus for ver- ifying whether core accretion coupled to migration is indeed the best option for forming close-in ...
15
HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars
... reject hot Jupiters, they note that their conclusion regarding the potential existence of two separate popula- tions still stands if those planets are included, and therefore we can place our new ...
18