Orientation of the cores of hybrid morphology radio sources

被引:11
作者
Ceglowski, M. [1 ]
Gawronski, M. P. [1 ]
Kunert-Bajraszewska, M. [1 ]
机构
[1] Nicholas Copernicus Univ, Torun Ctr Astron, PL-87100 Torun, Poland
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
galaxies: active; galaxies: jets; galaxies: nuclei; LUMINOSITY COMPACT SOURCES; ACTIVE GALACTIC NUCLEI; BL LACERTAE OBJECTS; FR-I; RELATIVISTIC JETS; VLBI OBSERVATIONS; LOUD AGN; 1.4; GHZ; GALAXIES; SAMPLE;
D O I
10.1051/0004-6361/201220544
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. The FR I/FR II dichotomy is a much debated issue in the astrophysics of extragalactic radio sources. Study of the properties of HYbrid MOrphology Radio Sources (HYMORS) may bring crucial information and lead to a step forward in understanding the origin of FR I/FR II dichotomy. HYMORS are a rare class of double-lobed radio sources where each of the two lobes clearly exhibits a different FR morphology. This article describes follow-up high resolution VLBA observations of the five discovered by us HYMORS. The main aim of the observations was to answer the questions of whether the unusual radio morphology is connected to the orientation of objects towards the observer. Methods. The milliarcsecond-scale structures are good probes of the galactic medium, the possible asymmetries, and orientation of the central engines of the sources. We obtained the high resolution radio maps of five hybrid radio morphology objects with the VLBA at C-band and L-band. Results. The cores of all five sources have been detected at both radio bands. Two of them revealed milliarcsecond core-jet structures, the next two objects showed hints of parsec-scale jets, and the last one remained point-like at both frequencies. Conclusions. We compared properties of observed milliarcsecond structures of hybrid sources with the larger scale ones previously detected with the VLA. We find that on both scales the fluxes of their central components are similar, which may indicate the lack of additional emission in the proximity of the nucleus. This suggests that jets present on the similar to 1-10 kpc scale in those objects are FR II-like. When possible, the detected core-jet structures were used for estimating the core's spatial orientation. The result is that neither the FRI-like nor the FRII-like side is preferred, which may suggest that no specific spatial orientation of HYMORS is required to explain their radio morphology. Their estimated viewing angles indicate they are unbeamed objects. The 178/151 MHz luminosity of observed HYMORS exceed the traditional FR I/FR II break luminosity, indicating they have radio powers similar to FR IIs.
引用
收藏
页数:6
相关论文
共 46 条
  • [1] IS EVERY QUASAR BEAMED
    BARTHEL, PD
    [J]. ASTROPHYSICAL JOURNAL, 1989, 336 (02) : 606 - 611
  • [2] The VLBA Calibrator Survey - VCSI
    Beasley, AJ
    Gordon, D
    Peck, AB
    Petrov, L
    MacMillan, DS
    Fomalont, EB
    Ma, C
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2002, 141 (01) : 13 - 21
  • [3] On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties
    Best, P. N.
    Heckman, T. M.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 421 (02) : 1569 - 1582
  • [4] RELATIVISTIC JETS AND THE FANAROFF-RILEY CLASSIFICATION OF RADIO GALAXIES
    BICKNELL, GV
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1995, 101 (01) : 29 - 39
  • [5] The deceleration of relativistic jets by entrainment
    Bowman, M
    Leahy, JP
    Komissarov, SS
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1996, 279 (03) : 899 - 914
  • [6] An optical spectroscopic survey of the 3CR sample of radio galaxies with z < 0.3 II. Spectroscopic classes and accretion modes in radio-loud AGN
    Buttiglione, S.
    Capetti, A.
    Celotti, A.
    Axon, D. J.
    Chiaberge, M.
    Macchetto, F. D.
    Sparks, W. B.
    [J]. ASTRONOMY & ASTROPHYSICS, 2010, 509
  • [7] A SAMPLE OF POWERFUL RADIO-SOURCES FOR VLBI STUDIES
    CAWTHORNE, TV
    SCHEUER, PAG
    MORISON, I
    MUXLOW, TWB
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1986, 219 (04) : 883 - 893
  • [8] Fanaroff B. L., 1974, MON NOT R ASTRON SOC, V167, P31
  • [9] Hybrid morphology radio sources from the FIRST survey
    Gawronski, MP
    Marecki, A
    Kunert-Bajraszewska, M
    Kus, AJ
    [J]. ASTRONOMY & ASTROPHYSICS, 2006, 447 (01): : 63 - U47
  • [10] The dividing line between FR I and FR II radio-galaxies
    Ghisellini, G
    Celotti, A
    [J]. ASTRONOMY & ASTROPHYSICS, 2001, 379 (01): : L1 - L4