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HD 202628
Pushing the Limits of the Coronagraphic Occulters on Hubble Space Telescope/Space Telescope Imaging Spectrograph
Poster Abstracts
Peter Plavchan
New Metallicity Calibration Down to [Fe/H]=−2.75
121012-AAS-221 Program-14-ALL, Page 253 @ Preflight
Chromospherically Young, Kinematically Old Stars
Observations, Modeling and Theory of Debris Discs
Feasibility of Transit Photometry of Nearby Debris Discs
Cycle 21 Approved Programs
High-Resolution Spectroscopy of Some Active Southern Stars
269 — 12 May 2015 Editor: Bo Reipurth (
[email protected]
) List of Contents
Non-LTE Analysis of K I in Late-Type Stars? Henrique Reggiani1,2, Anish M
From Scattered-Light to Millimeter Emission: a Comprehensive View of the Gyr-Old System of HD 202628 and Its Eccentric Debris Ring
SKARPS: the Search for Kuiper-‐Belts Around Radial-‐Velocity Planet Stars
The Astronomical Journal, 149:86 (7Pp), 2015 February Doi:10.1088/0004-6256/149/2/86 © 2015
Numerical Predictions for Planets in the Debris Discs of HD 202628 and HD 207129
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
Pushing the Limits of the Coronagraphic Occulters on Hubble Space Telescope/Space Telescope Imaging Spectrograph
Top View
Arxiv:1707.07051V1 [Astro-Ph.SR] 21 Jul 2017 E Nteyugs Lses(Age Clusters Youngest the in Dex E Ncutr Le Hntesn H [Ba the Sun
Astronomy Astrophysics
Peter Plavchan
Shallow Extra Mixing in Solar Twins Inferred from Be Abundances ⋆
Apocenter Glow in Eccentric Debris Disks: Implications for Fomalhaut And
Planet Formation and Evolution 2019
Project Final Report
Cycle 21 Abstract Catalog (Based on Phase I Submissions)
Phase 2, *AND* the SIAF Locations of the Aperture Fiducial We Determined in GO 12923 Is Yet to Be Populated in SIAF.Dat and Flowed Down to the Ground System
Observing Exoplanets with the James Webb Space Telescope
45Th Annual Meeting Division for Planetary Sciences Denver, Colorado | 6-11 October 2013
Debris Disks: Structure, Composition, and Variability Arxiv:1802.04313V1 [Astro-Ph.EP] 12 Feb 2018
Statistical Modelling of Resolved Debris Discs