Understanding BL Lacertae objects: Structural and kinematic mode changes in the BL Lac object PKS 0735+178

Astronomy and Astrophysics

Volumn 515, Issue 11, 2010, Pages

  Britzen, S ^a   Witzel, A ^a   Gong, B P ^b   Zhang, J W ^b   Krishna, G ^c   Goyal, A ^d   Aller, M F ^e   Aller, H D ^e   Zensus, J A ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b HUAZHONG UNIVERSITY OF SCIENCE AND TECHNOLOGY   (China)

^c NATIONAL CENTRE FOR RADIO ASTROPHYSICS   (India)

^d ARYABHATTA RESEARCH INSTITUTE OF OBSERVATIONAL SCIENCES ARIES   (India)

^e UNIVERSITY OF MICHIGAN   (United States)

Author keywords

BL Lacertae objects: individual: PKS 0735+178; Radio continuum: galaxies; Techniques: interferometric

Indexed keywords

GALAXIES; INTERFEROMETRY; MORPHOLOGY; OPTICAL CORRELATION; OPTICAL PROPERTIES; RADIO ASTRONOMY;

AMBIENT MEDIUM; BALLISTIC MOTIONS; BL LACERTAE OBJECTS; EMISSION PROCESS; FLUX DENSITIES; GAUSSIANS; KINEMATIC PROPERTIES; LIGHT CURVES; LONG BASELINE ARRAY; MOTION CHARACTERISTICS; OPTICAL LIGHT; RADIO CONTINUUM: GALAXIES; RADIO FLUX; RADIO JET; RIDGE LINES; SIMILAR PATTERN; STATIONARITY; STRUCTURAL MODES; SUPERLUMINAL; VERY LONG BASELINE INTERFEROMETRY; VIEWING ANGLE;

KINEMATICS;

EID: 77953632068     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913685     Document Type: Article

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