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Volumn 532, Issue , 2011, Pages

The mean infrared emission of Sagittarius A*

Author keywords

Black hole physics; Galaxy: center; Instrumentation: adaptive optics; Instrumentation: high angular resolution

Indexed keywords

ANCHOR POINT; AT-WAVELENGTH; BLACK HOLE PHYSICS; BLACK HOLES; FLUX DENSITIES; GALAXY: CENTER; HIGH-FREQUENCY SIDE; IMAGING DATA; IMAGING QUALITY; INFRARED EMISSIONS; INSTRUMENTATION: ADAPTIVE OPTICS; INSTRUMENTATION:HIGH ANGULAR RESOLUTION; MASSIVE BLACK HOLES; MILKY WAYS; MODEL PARAMETERS; NOVEL TECHNIQUES; POINT SOURCES; SPECKLE IMAGING; TERA HERTZ; THEORETICAL MODELS; TIME-AVERAGED; TIME-SCALES; UPPER LIMITS;

EID: 79960788847     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116994     Document Type: Review
Times cited : (92)

References (63)
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    • Lutz, D. 1999, in ESA Spec. Publ., 427, The Universe as Seen by ISO, ed. P. Cox, & M. Kessler, 623
    • (1999) ESA Spec. Publ. , vol.427 , pp. 623
    • Lutz, D.1
  • 51
    • 1842470129 scopus 로고    scopus 로고
    • ed. P. L. Wizinowich, & D. Bonaccini
    • Rousset, G., Lacombe, F., Puget, P., et al. 2003, in SPIE Conf. Ser., 4839, ed. P. L. Wizinowich, & D. Bonaccini, 140
    • (2003) SPIE Conf. Ser. , vol.4839 , pp. 140
    • Rousset, G.1    Lacombe, F.2    Puget, P.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.