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HR 8799 d
Naming the Extrasolar Planets
GEMINI PLANET IMAGER SPECTROSCOPY of the HR 8799 PLANETS C and D
Planet Searching from Ground and Space
The Formation Mechanism of Gas Giants on Wide Orbits
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Radial Velocity of Directly Imaged Planets Jean-Baptiste Ruffio, OSIRIS: Quinn M
The LEECH Exoplanet Imaging Survey. Further Constraints on the Planet Architecture of the HR 8799 System?
DIRECT DETECTION and ORBITAL ANALYSIS of the EXOPLANETS HR 8799 Bcd from ARCHIVAL 2005 KECK/NIRC2 DATA
Enrichment of the HR 8799 Planets by Minor Bodies and Dust Frantseva, K.; Mueller, M.; Pokorný, P.; Van Der Tak, F
GEMINI PLANET IMAGER SPECTROSCOPY of the HR 8799 PLANETS C and D
VLT/NACO Astrometry of the HR 8799 Planetary System⋆
A Possible Architecture of the Planetary System HR 8799
Modelling the Inner Debris Disc of HR 8799
CHAPTER 7 the NATURE of EXOPLANETARY SYSTEMS Now That the Various Methods of Detecting Exoplanets Have Been Described, We Turn to the Results of the Various Searches
Spatially Resolved Spectroscopy of the Exoplanet HR 8799 C∗
Fa.Ce-Qn, and Coplanar Orbits Are Incon
FIRST LIGHT LBT AO IMAGES of HR 8799 Bcde at 1.6 and 3.3 Μm: NEW DISCREPANCIES BETWEEN YOUNG PLANETS and OLD BROWN DWARFS∗
Astronomical Science As Is Apparent from the Many H Many the from Apparent Is As H Large Avery Has NGC 7793 Distance
Top View
1 Bruna Contro1,*, Rob Wittenmyer1,2,3, Jonti Horner2,3
Enrichment of the HR 8799 Planets by Minor Bodies and Dust K
Towards a Dynamics-Based Estimate of the Extent of HR 8799'S
New Constraints on the HR 8799 Planetary System from Mid-Infrared Direct Imaging ?
Arxiv:1808.02454V1 [Astro-Ph.EP] 7 Aug 2018
Direct Imaging of Exoplanets: Remote Sensing of Planetary Systems And
Reconnaissance of the Hr 8799 Exosolar System. I. Near-Infrared Spectroscopy
Formation and Evolution of Planetary Systems: the Impact of High-Angular
Thermal Infrared Mmtao Observations of the Hr 8799 Planetary System∗
Arxiv:1311.2085V2
Masses, Radii, and Cloud Properties of the HR 8799 Planets