A spectroscopic study of the blue stragglers in M67
- Author
- LIU, G. Q1 2 ; DENG, L1 ; CHAVEZ, M3 ; BERTONE, E3 ; HERRERO DAVO, A4 ; MATA-CHAVEZ, M. D5
[1] NAOC -National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
[2] GUCAS-Graduate University of Chinese Academy of Sciences, Beijing 100049, China
[3] INAOE -Institute Nacional de Astrofí sica, Óptica y Electrónica, Luis Enrique Erro I, 72840 Tonantzintia, Puebla, Mexico
[4] IAC -Instituto de Astrofi ca de Canarias, 38205 La Laguna, Tenerife, Spain
[5] Departamento de Fisica, CUCEI, Universidad de Guadalajara, Blvd. Marcelino Garcia Barragan 1412, Guadalajara, Jalisco, Mexico - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 390, Num 2, pp 665-674, 10 p ; ref : 1/2 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- Hertzsprung-Russell (HR) diagram blue stragglers open clusters and associations: individual: M67
- Keyword (fr)
- Amas galactique Amas ouvert Amas stellaire Blue straggler Diagramme HR Gravité surface Observation spectrophotométrique Propriété spectrale Spectre optique Type spectral
- Keyword (en)
- Galactic cluster Open clusters Star clusters Blue stragglers Hertzsprung Russel diagram Surface gravity Spectrophotometric observation Spectral properties Optical spectrum Spectral type
- Keyword (es)
- Conglomerado galáctico Diagrama HR Observación espectrofotométrica Propiedad espectral Espectro óptico Tipo espectral
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20755489
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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