First VLTI infrared spectro-interferometry on GCIRS 7. Characterizing the prime reference source for Galactic center observations at highest angular resolution

Astronomy and Astrophysics

Volumn 487, Issue 1, 2008, Pages 413-418

  Pott, J U ^a,b,c   Eckart, A ^c   Glindemann, A ^d   Kraus, S ^e   Schodel R ^f   Ghez, A M ^b   Woillez, J ^a   Weigelt, G ^e  

^a W M KECK OBSERVATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF COLOGNE   (Germany)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Galaxy: center; Infrared: stars; Instrumentation: interferometers; ISM: dust, extinction; Stars: supergiants; Stars: winds, outflows

Indexed keywords

ABSORPTION; ASTRONOMY; DUST; GEODETIC SATELLITES; IMAGING TECHNIQUES; INFRARED DEVICES; INTERFEROMETRY; OPTICAL PROPERTIES; OPTICAL TELESCOPES; PHOTOGRAPHY; SENSITIVITY ANALYSIS; SILICATES; STARS; TELESCOPES; VISIBILITY;

2 MICRON; ANGULAR RESOLUTIONS; DUST COMPOSITION; FIELD FACILITIES; FRINGE DETECTION; GALACTIC CENTER (GC); INFRARED (IR); INTERFEROMETRIC PHASE; LARGE APERTURES; MASSIVE BLACK HOLES; OPTICAL (PET) (OPET); PHASE REFERENCING; PHASE-REFERENCING; REFERENCE SOURCES; TELESCOPE ARRAY (TA); WAVE FRONTS; WAVELENGTH COVERAGE; WAVELENGTH DEPENDENCE;

LAWS AND LEGISLATION;

EID: 48249090888     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809829     Document Type: Article

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