The Galactic O-Star Spectroscopic Survey : I. Classification system and bright northern stars in the Blue-Violet at R ∼ 2500

We present the first installment of a massive spectroscopic survey of Galactic O stars, based on new, high signal-to-noise ratio, R ∼ 2500 digital observations from both hemispheres selected from the Galactic O-Star Catalog of Maíz Apellniz etal. and Sota etal. The spectral classification system is...

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Detalles Bibliográficos
Autores: Sota, Alfredo, Maíz Apellániz, Jesús, Walborn, Nolan Revere, Alfaro, Emilio J., Barbá, Rodolfo Héctor, Morrell, Nidia Irene, Gamen, Roberto Claudio, Arias, Julia Inés
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2011
País:Argentina
Institución:Universidad Nacional de La Plata
Repositorio:SEDICI (UNLP)
Idioma:inglés
OAI Identifier:oai:sedici.unlp.edu.ar:10915/83946
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/83946
Access Level:acceso abierto
Palabra clave:Ciencias Astronómicas
binaries: general
stars: early-type
stars: emission-line, Be
stars: Wolf-Rayet
surveys
Descripción
Sumario:We present the first installment of a massive spectroscopic survey of Galactic O stars, based on new, high signal-to-noise ratio, R ∼ 2500 digital observations from both hemispheres selected from the Galactic O-Star Catalog of Maíz Apellniz etal. and Sota etal. The spectral classification system is rediscussed and a new atlas is presented, which supersedes previous versions. Extensive sequences of exceptional objects are given, including types Ofc, ON/OC, Onfp, Of?p, Oe, and double-lined spectroscopic binaries. The remaining normal spectra bring this first sample to 184 stars, which is close to complete to B = 8 and north of δ = -20° and includes all of the northern objects in Maíz Apellniz etal. that are still classified as O stars. The systematic and random accuracies of these classifications are substantially higher than previously attainable, because of the quality, quantity, and homogeneity of the data and analysis procedures. These results will enhance subsequent investigations in Galactic astronomy and stellar astrophysics. In the future, we will publish the rest of the survey, beginning with a second paper that will include most of the southern stars in Maíz Apellniz etal.