A proper motion study of the Lupus clouds using Virtual Observatory tools

2011/03/14 by Belén López Martí, F. Jiménez-Esteban, Francisco Jiménez-Esteban +2 · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Geography #Physics #Proper motion #Stars #Stellar, planetary, and galactic studies #Systemic lupus erythematosus #Virtual observatory #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201016377

Accepted in A&A

arxiv created 2011/03/14 · openalex publication_date 2011/03/14 · arxiv updated 2015/05/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The Lupus dark cloud complex is a well-known, nearby low-mass star-forming region, probably associated with the Gould Belt. In recent years, the number of stellar and substellar Lupus candidate members has been remarkably increased thanks to the Cores to Disks (c2d) Spitzer Legacy Program and other studies. However, most of these newly discovered objects still lack confirmation that they belong to the dark clouds.

Citations

• Improved kinematics for brown dwarfs and very low-mass stars in Chamaeleon I and a discussion of brown dwarf formation
• Stellar, brown dwarf and multiple star properties from hydrodynamical simulations of star cluster formation
• JHKLM photometry - Standard systems, passbands, and intrinsic colors
• Disk Frequencies and Lifetimes in Young Clusters
• The Two Micron All Sky Survey (2MASS)
• New Low‐Mass Stars and Brown Dwarfs with Disks in Lupus
• The NextGen Model Atmosphere Grid for \documentclassaastex \usepackageamsbsy \usepackageamsfonts \usepackageamssymb \usepackagebm \usepackagemathrsfs \usepackagepifont \usepackagestmaryrd \usepackagetextcomp \usepackageportland,xspace \usepackageamsmath,amsxtra \usepackage[OT2,OT1]fontenc \newcommand\cyr \renewcommand\rmdefaultwncyr \renewcommand\sfdefaultwncyss \renewcommand\encodingdefaultOT2 \normalfont \selectfont \DeclareTextFontCommand\textcyr\cyr \pagestyleempty \DeclareMathSizes10976 \begindocument \landscape 3000≤ T_eff ≤ 10,000 \enddocument K

Cited by

• Proper motions of young stars in Chamaeleon
• Lupus DANCe

Related

• Star Formation In Bright-rimmed Clouds. I. Millimeter And Submillimeter Molecular Line Surveys
• Measuring Nearby Star Forming Regions with the VLBA: from the Distance to the Dynamics
• Low-Mass Stars in the Sloan Digital Sky Survey: Galactic Structure,\n Kinematics, and the Luminosity Function
• Mass Transport Processes and their Roles in the Formation, Structure, and Evolution of Stars and Stellar Systems
• Cold Dark Clouds: The Initial Conditions for Star Formation