2018ApJ...858...83C


Query : 2018ApJ...858...83C

2018ApJ...858...83C - Astrophys. J., 858, 83-83 (2018/May-2)

Giant double radio source DA 240: purveyor of galaxies.

CHEN R.-R., STROM R. and PENG B.

Abstract (from CDS):

Galaxies of stars are building blocks of the baryonic universe. Their composition, structure, and kinematics have been well studied, but details of their origins remain sketchy. The collapse of gas clouds, induced by external forces whereby gravity overcomes internal pressure to form stars, is the likely starting point. Among the perturbing initiators of galaxy formation, radio source beams (jets) are quite effective. Typically, a beam may spawn one galaxy, though instances of several aligned with the radio axis are known. Recently, we found an impressive 14 companions in the lobes of the giant radio galaxy DA 240, which we argue formed as the result of jet instigation. This conclusion is bolstered by the fact that the galaxy groups display Z-shaped symmetry with respect to the radio axis. There is some evidence for star formation among the aligned companions. We also conclude that galaxy alignments at low redshift may derive from line-emitting gas observed in radio components of high-redshift galaxies.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): galaxies: active - galaxies: formation - galaxies: individual: DA 240 - galaxies: jets

Simbad objects: 28

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Number of rows : 28
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 NGC 375 AG? 01 07 05.9200285896 +32 20 53.197225548   16.5       ~ 59 0
2 NGC 383 AGN 01 07 24.9647814840 +32 24 45.132586200   13.6 12.14     ~ 821 3
3 NGC 541 AGN 01 25 44.3069825040 -01 22 46.086331044 13.42 13.03 12.08     ~ 219 2
4 3C 171.0 Sy2 06 55 14.7385158451 +54 08 57.427918985   19.94 19.08     ~ 264 1
5 2MASX J07463016+5538440 EmG 07 46 30.1866456648 +55 38 44.064494664           ~ 4 0
6 [PSW2004] 37 G 07 46 53.0 +55 41 16       14.4   ~ 2 0
7 2MASS J07470750+5543453 G 07 47 07.4938002792 +55 43 45.206824368           ~ 3 0
8 [PSW2004] 5 HII 07 47 32.90 +55 41 48.2           ~ 2 0
9 [PSW2004] 38 G 07 47 33.5 +55 41 00       15.6   ~ 2 0
10 2MASX J07473549+5541185 GiC 07 47 35.4492296112 +55 41 18.458288772           ~ 6 0
11 [PSW2004] 7 HII 07 47 45.94 +55 46 41.4           ~ 2 0
12 2MASX J07475505+5546283 EmG 07 47 55.1053120344 +55 46 28.094869848           ~ 4 0
13 2MASX J07475776+5545093 G 07 47 57.7114117680 +55 45 09.584426448           ~ 2 0
14 Z 262-29 rG 07 48 36.8495635584 +55 48 58.722052320   15.2 15.2     ~ 33 1
15 [PSW2004] 33 G 07 49 00 +55 55.1           ~ 1 0
16 2MASS J07491348+5556491 HII 07 49 13.49 +55 56 49.2           ~ 3 0
17 [VV2006] J074924.5+555814 QSO 07 49 24.5472685296 +55 58 13.323942444           ~ 10 0
18 MCG+09-13-064 G 07 49 37.9026272304 +55 52 44.145172416   18       ~ 5 0
19 4C 56.16 rG 07 49 48.077 +55 54 19.45           ~ 176 1
20 Z 262-33 Sy2 07 49 58.4867093496 +55 55 27.614020224   15.4       ~ 26 0
21 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
22 3C 277.3 BLL 12 54 12.0071453880 +27 37 33.952663740   15.94       ~ 379 1
23 6C 131905+425044 Sy2 13 21 17.813 +42 35 15.38   16.86 16.23     ~ 282 1
24 VV 204 SyG 15 04 57.1195361592 +26 00 58.455780156   15.24       ~ 299 1
25 3C 314.1 rG 15 10 23.1 +70 45 54   17       ~ 92 0
26 MCG+01-43-006 SyG 16 51 07.9886687784 +04 59 35.547131472     18.25     ~ 502 1
27 Z 173-14 Sy1 18 35 03.3896172576 +32 41 46.855964616   16.50 15.39 10.50   ~ 688 1
28 Z 114-25 rG 18 38 26.25747 +17 11 49.6210           ~ 205 2

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