Results 71 to 80 of about 53,007 (245)
A Third Star in the HAT-P-7 System and a New Dynamical Pathway to Misaligned Hot Jupiters
The Astrophysical JournalThe retrograde orbit of the hot Jupiter HAT-P-7b is suggestive of high-eccentricity (high-e) migration caused by dynamical interactions with a massive companion.
Eritas Yang, Yubo Su, Joshua N. Winn
doaj +1 more source
The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey [PDF]
, 2022 David G. Jackson +37 more
openalex +1 more source
Hot Jupiters from secular planet–planet interactions [PDF]
Nature, 2011 accepted for publication by Nature, 3 figures (version after proof - some typos corrected)
Naoz, Smadar +4 more
openaire +3 more sources
Polymer International, EarlyView.Fullerene particles were incorporated with CF‐reinforced acrylonitrile–butadiene–styrene terpolymer (ABS) matrix at three different compositions by a melt‐compounding process. These insights are crucial for the optimization of conductive hybrid composites for various applications.
Alinda Öyku Akar +4 more
wiley +1 more source
Planets spinning up their host stars: a twist on the age-activity relationship
, 2013 It is a long-standing question in exoplanet research if Hot Jupiters can influence the magnetic activity of their host stars. While cool stars usually spin down with age and become inactive, an input of angular momentum through tidal interaction, as seen
Poppenhaeger, K., Wolk, S. J.
core +1 more source
Formation of Ultra-short-period Planets in Hot Jupiter Systems: Application to WASP-47
The Astrophysical Journal LettersThe WASP-47 system is notable as the first known system hosting both inner and outer low-mass planetary companions around a hot Jupiter, with an ultra-short-period (USP) planet as the innermost planetary companion.
Su Wang +4 more
doaj +1 more source
Hot Jupiter secondary eclipses measured by Kepler
EPJ Web of Conferences, 2011 Hot-Jupiters are known to be dark in visible bandpasses, mainly because of the alkali metal absorption features. The outstanding quality of the Kepler mission photometry allows a detection (or non-detection upper limits on) giant planet secondary ...
Seager S., Demory B.-O.
doaj +1 more source
Thermosphere and exosphere of hot Jupiters [PDF]
Proceedings of the International Astronomical Union, 2008 AbstractHere we describe the observations and the resulting constraints on the upper atmosphere (thermosphere and exosphere) of hot Jupiters. In particular, observations and theoretical modeling of hot-Jupiter evaporation are described. The observations allowed the discovery that the planet orbiting HD209458 has an extended atmosphere of escaping ...
openaire +2 more sources
steel research international, EarlyView.This work demonstrates that replacing Ti with Nb in maraging steel forms nanoscale Nb–Mo particles along boundaries, strengthening the alloy without relying on Ti phases. Heat‐treatment tuning promotes uniform crystal orientation and balanced grain boundaries, enabling strong yet ductile behavior.
Mohamad Masoumi +14 more
wiley +1 more source
Atmospheric Characterization of the Hot Jupiter Kepler-13Ab [PDF]
, 2014 Kepler-13Ab (= KOI-13.01) is a unique transiting hot Jupiter. It is one of very few known short-period planets orbiting a hot A-type star, making it one of the hottest planets currently known.
Agol, Eric +14 more
core +4 more sources