2007PASJ...59..703D


Query : 2007PASJ...59..703D

2007PASJ...59..703D - Publ. Astron. Soc. Jap., 59, 703-709 (2007/August-0)

Japanese VLBI network observations of radio-loud narrow-line Seyfert 1 galaxies.

DOI A., FUJISAWA K., INOUE M., WAJIMA K., NAGAI H., HARADA K., SUEMATSU K., HABE A., HONMA M., KAWAGUCHI N., KAWAI E., KOBAYASHI H., KOYAMA Y., KUBOKI H., MURATA Y., OMODAKA T., SORAI K., SUDOU H., TAKABA H., TAKASHIMA K., TAKEDA K., TAMURA S. and WAKAMATSU K.-I.

Abstract (from CDS):

begin{HTML}We performed phase-reference very long baseline interferometry (VLBI) observations on five radio-loud narrow-line Seyfert 1 galaxies (NLS1s) at 8.4 GHz with the Japanese VLBI Network. Each of the five targets (RXS J08066+7248, RXS J16290+4007, RXS J16333+4718, RXS J16446+2619, and B3 1702+457) in milli-Jansky levels were detected and unresolved in milli-arcsecond resolutions, i.e., with brightness temperatures higher than 107K. The nonthermal processes of active galactic nucleus activity, rather than starbursts, are predominantly responsible for the radio emissions from these NLS1s. Out of the nine known radio-loud NLS1s, including those chosen for this study, we found that the four most radio-loud objects exclusively have inverted spectra. This suggests a possibility that these NLS1s are radio-loud due to Doppler beaming, which can apparently enhance both the radio power and the spectral frequency.

Abstract Copyright: ∼

Journal keyword(s): galaxies: active - galaxies: jets - galaxies: Seyfert - radio continuum: galaxies - techniques: interferometric

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 2MASS J00445912+1921412 Sy1 00 44 59.1277028184 +19 21 41.244352128     16.1     ~ 37 0
2 2MASS J01341690-4258262 Sy1 01 34 16.9072341600 -42 58 26.223391344   18.17 17.30 16.71   ~ 81 1
3 M 77 Sy2 02 42 40.7091669408 -00 00 47.859690204 9.70 9.61 8.87 10.1 9.9 ~ 4897 2
4 QSO B0558-5026 BLL 05 59 47.3916612936 -50 26 52.025952120   15.18 14.97     ~ 307 1
5 NVSS J075445+714056 Rad 07 54 45.49923431 +71 40 56.7358292           ~ 12 1
6 LEDA 3095785 Sy1 08 06 38.9574958032 +72 48 20.403834696   15.9       ~ 28 1
7 8C 0802+733 Bla 08 08 16.49154497 +73 15 11.9897583       20.30   ~ 36 1
8 QSO J0948+0022 Bla 09 48 57.32005819 +00 22 25.5596984   18.85 18.61 18.17   ~ 350 2
9 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1507 1
10 SN 1988Z SN* 10 51 50.10 +16 00 00.5   16.8       SNIIn 385 1
11 NGC 4253 Sy1 12 18 26.5163572920 +29 48 46.531535472   14.34 13.57     ~ 1106 1
12 NGC 5506 Bla 14 13 14.8761010056 -03 12 27.556909272   15.25 14.38     ~ 1173 1
13 7C 162123.89+391619.00 Bla 16 23 07.6225499136 +39 09 32.410546992   17.41 17.21 16.10   ~ 97 1
14 4C 41.32 Bla 16 25 57.66971273 +41 34 40.6292008     22 21.73   ~ 171 1
15 [VV98] J162837.6+473410 QSO 16 28 37.5052485168 +47 34 10.423781868   21.39 20.85     ~ 38 1
16 2MASS J16290130+4007599 Bla 16 29 01.3106358000 +40 07 59.905936776   18.23 18.00 17.2   ~ 111 0
17 2MASX J16332357+4718588 Sy1 16 33 23.5812109560 +47 18 58.936241628   17.77 17.35     ~ 88 1
18 4C 47.44 Bla 16 37 45.13055568 +47 17 33.8311081   17.5   18.69   ~ 183 1
19 6C 163852+395305 Bla 16 40 29.63277140 +39 46 46.0284071   18.4 19.37 18.75   ~ 336 2
20 7C 164055.20+534559.00 Sy1 16 42 00.5603239320 +53 39 50.603024736   17.82 17.04     ~ 16 1
21 [VV2000] J164240.4+252307 Bla 16 42 40.4116160856 +25 23 07.683525492   18.82 18.66 17.5   ~ 59 1
22 QSO J1644+2619 Bla 16 44 42.5339200680 +26 19 13.227002976   18.80 18.42     ~ 114 1
23 6C 170204+454510 Sy1 17 03 30.3824218008 +45 40 47.166180564   16.0       ~ 170 2
24 NVSS J170348+455936 Rad 17 03 48.299 +45 59 35.24           ~ 3 1
25 4C 45.34 Bla 17 07 17.7533536464 +45 36 10.552931460   17.18 17.01 17   ~ 79 1
26 Z 495-18 Sy1 22 42 39.3363009144 +29 43 31.302092640   14.86 14.16     ~ 748 1

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