The pre-main-sequence binary HK Ori: Spectro-astrometry and EXPORT data

Monthly Notices of the Royal Astronomical Society

Volumn 353, Issue 2, 2004, Pages 697-704

  Baines, D ^a,b   Oudmaijer, R D ^a   Mora, A ^c   Eiroa, C ^c   Porter, John M ^d   Merin B ^e   Montesinos, B ^e,f   De Winter, D ^g   Cameron, A ^h   Davies, J K ⁱ   Deeg, H J ^j   Ferlet, R ^k   Grady, C A ^l   Harris, A W ^m   Hoare, M G ^a   Horne, K ^h   Lumsden, S L ^a   Miranda, L F ^f   Penny, A ⁿ   Quirrenbach, A ^o  

^a UNIVERSITY OF LEEDS   (United Kingdom)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^d LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^e CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^f INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^g TNO   (Netherlands)

^h UNIVERSITY OF ST ANDREWS   (United Kingdom)

ⁱ UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^j INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^k INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^l NASA GODDARD SPACE FLIGHT CENTER   (United States)

^m GERMAN AEROSPACE CENTER DLR   (Germany)

ⁿ RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^o LEIDEN UNIVERSITY   (Netherlands)

more..

Author keywords

Binaries: spectroscopic; Stars: individual: HK Ori; Stars: pre main sequence; Techniques: spectroscopic

Indexed keywords

BINARIES: SPECTROSCOPIC; DATA BASE; HIGH QUALITY; SPECTRA'S; STAR: INDIVIDUAL: HK ORI; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: PRE-MAIN SEQUENCE; T TAURI STARS; TECHNIQUES: SPECTROSCOPIC;

STARS;

EID: 4544233264     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08104.x     Document Type: Article

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