Mid-infrared interferometry of the Mira variable RR Sco with the VLTI MIDI instrument

Astronomy and Astrophysics

Volumn 429, Issue 3, 2005, Pages 1057-1067

  Ohnaka, K ^a   Bergeat, J ^b   Driebe, T ^a   Graser, U ^c   Hofmann, K H ^a   Kohler R ^c   Leinert, Ch ^c   Lopez, B ^d   Malbet, F ^e   Morel, S ^f   Paresce, F ^g   Perrin, G ^h   Preibisch, Th ^a   Richichi, A ^g   Schertl, D ^a   Scholler M ^f   Sol, H ^h   Weigelt, G ^a   Wittkowski, M ^g  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b OBSERVATOIRE DE LYON   (France)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^d UNIVERSITÉ CÔTE D'AZUR   (France)

^e LABORATOIRE D ASTROPHYSIQUE   (France)

^f EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^h OBSERVATOIRE DE PARIS   (France)

Author keywords

Infrared: stars; Stars: AGB and post AGB; Stars: circumstellar matter; Stars: individual: RR Sco; Stars: mass loss; Techniques: interferometric

Indexed keywords

ADSORPTION; DUST; INTERFEROMETRY; SPECTRUM ANALYSIS; TELESCOPES; THERMAL EFFECTS;

INFRARED: STARS; POST-AGB; RR SCO; STARS: AGB; STARS: CIRCUMSTELLAR MATTER; STARS: INDIVIDUAL; STARS: MASS-LOSS; TECHNIQUES: INTERFEROMETRIC;

ASTROPHYSICS;

EID: 19944428392     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041052     Document Type: Article

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