English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/182541
Share/Impact:
Statistics
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:
Title

Lucky Spectroscopy, an equivalent technique to Lucky Imaging. Spatially resolved spectroscopy of massive close visual binaries using the William Herschel Telescope

AuthorsMaíz Apellániz, Jesús ; Barbá, R. H.; Simón-Díaz, S.; Sota Ballano, Alfredo ; Trigueros Páez, E.; Caballero, J. A.; Alfaro, Emilio J.
KeywordsMassive-techniques
Visual-methods
Spectroscopic-binaries
Spectroscopic
Binaries
Data analysis-stars
Early-type-stars
Issue Date2018
PublisherEDP Sciences
CitationAstronomy and Astrophysics 615: A161 (2018)
AbstractContext. Many massive stars have nearby companions whose presence hamper their characterization through spectroscopy. Aims: We want to obtain spatially resolved spectroscopy of close massive visual binaries to derive their spectral types. Methods: We obtained a large number of short long-slit spectroscopic exposures of five close binaries under good seeing conditions. We selected those with the best characteristics, extracted the spectra using multiple-profile fitting, and combined the results to derive spatially separated spectra. Results: We demonstrate the usefulness of Lucky Spectroscopy by presenting the spatially resolved spectra of the components of each system, in two cases with separations of only 0.''3. Those are ¿ Ori Aa+Ab (resolved in the optical for the first time) and ¿ Ori AaAb+B (first time ever resolved). We also spatially resolve 15 Mon AaAb+B, ¿ Ori AaAb+B (both previously resolved with GOSSS, the Galactic O-Star Spectroscopic Survey), and ¿ Ori AaAb+B, a system with two spectroscopic B+B binaries and a fifth visual component. The systems have in common that they are composed of an inner pair of slow rotators orbited by one or more fast rotators, a characteristic that could have consequences for the theories of massive star formation.© 2018 EDP Sciences. All rights reserved.
URIhttp://hdl.handle.net/10261/182541
Identifiersdoi: 10.1051/0004-6361/201832885
issn: 1432-0746
Appears in Collections:(IAA) Artículos
(CAB) Artículos
Files in This Item:
File Description SizeFormat 
IAA_2018_aa32885-18.pdf559,02 kBAdobe PDFThumbnail
View/Open
Show full item record
Review this work
 

Related articles:


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.