DUst around NEarby Stars. The survey observational results

2013/05/01 by C. Eiroa, J. P. Marshall, A. Mora +47 · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201321050

openalex publication_date 2013/05/01 · arxiv created 2013/05/06 · arxiv updated 2015/06/15 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and Edgeworth-Kuiper belts.

Citations

• Far‐Infrared Properties of M Dwarfs
• Debris Disks in Main‐Sequence Binary Systems
• Debris Disks around Sun‐like Stars
• The Planet‐Metallicity Correlation
• Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.
• New Debris Disks around Nearby Main‐Sequence Stars: Impact on the Direct Detection of Planets
• Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections
• Evolution of Debris Disks
• Validation of the new Hipparcos reduction
• Improved Age Estimation for Solar‐Type Dwarfs Using Activity‐Rotation Diagnostics
• Drizzle: A Method for the Linear Reconstruction of Undersampled Images
• Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Southern Sample

Cited by

• Analysis of the Herschel DEBRIS Sun-like star sample
• Mensa (constellation) [wikipedia]