2004BaltA..13..273L


Query : 2004BaltA..13..273L

2004BaltA..13..273L - Baltic Astronomy, 13, 273-279 (2004/February-0)

Astrophysical jets.

LIVIO M.

Abstract (from CDS):

The acceleration and collimation mechanisms of jets probably are the same in all the classes of astrophysical objects which exhibit them: active galactic nuclei, young stellar objects, massive X-ray binaries, low mass X-ray binaries, black hole X-ray transients, gamma-ray bursts, symbiotic systems, planetary nebulae, supersoft X-ray sources and possibly recurrent novae and pulsars. An attempt is made to identify the necessary ingredients for the acceleration and collimation mechanisms. Most likely, the jets are produced at the center of accretion disks and are accelerated and collimated hydromagnetically.

Abstract Copyright: ∼

Journal keyword(s): gamma-rays: bursts - accretion: accretion disks - stars: outflows

CDS comments: p.274: 1E 140.7-2942 is a misprint for 1E 1740.7-2942 ?

Simbad objects: 27

goto View the references in ADS

Number of rows : 27
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 V* QR And CV* 00 19 49.9252996176 +21 56 52.169584416   12.38 12.73 11.86   Ss 139 0
2 [EM98] DG Tau B cRN Y*O 04 27 02.66088 +26 05 30.4548           ~ 208 0
3 V* V1213 Tau Or* 04 31 37.5055489536 +18 12 24.383952396           K7 605 0
4 SV* HV 5682 XB* 05 13 50.7835871075 -69 51 47.483214339     16.566 16.606 16.62 ~ 321 0
5 HH 34 HH 05 35 31.30 -06 28 43.0     16     ~ 493 2
6 Haro 5-6 Y*O 05 37 22.5487551696 -02 59 36.407573988   16.47 15.06 14.13 13.15 ~ 12 0
7 2E 1550 XB* 05 43 34.1600044704 -68 22 22.191505716   15.9   17.2 16.54 ~ 332 0
8 EM* MWC 560 Sy* 07 25 51.2842107720 -07 44 08.084175396   10.01 9.70 10.60   M4ep+Beq 223 0
9 PN K 1-2 PN 08 57 45.9621412752 -28 57 36.577846476           ~ 125 1
10 MCG-05-23-016 Sy2 09 47 40.1332188528 -30 56 55.960779696   14.10 13.69 12.44   ~ 611 0
11 NGC 4151 Sy1 12 10 32.5759813872 +39 24 21.063527532   12.18 11.48     ~ 3938 2
12 M 106 Sy2 12 18 57.620 +47 18 13.39   9.14 8.41 8.11   ~ 2512 4
13 NGC 4261 LIN 12 19 23.2160630 +05 49 29.700024   13.92 12.87     ~ 1290 0
14 MCG-06-30-015 Sy1 13 35 53.7691256160 -34 17 44.160716796   13.89 13.61 8.9   ~ 1559 0
15 NGC 5458 HII 14 03 12.54647 +54 17 55.3700           ~ 11 1
16 WRAY 16-147 Sy* 14 11 52.0604355768 -51 26 24.187122024     14.20     ~ 240 1
17 V* BR Cir HXB 15 20 40.8532547060 -57 10 00.206639033   21.4 21.4     B5-A0I 849 1
18 V* V1033 Sco HXB 16 54 00.1423963019 -39 50 44.761701340       16.14   F3-6IV 1980 0
19 2E 3938 HXB 17 43 54.7 -29 44 44           ~ 693 1
20 NGC 6543 PN 17 58 33.4039587288 +66 37 58.750734000   11.09 11.28     [WC] 1197 2
21 3C 390.3 Bla 18 42 08.9904975672 +79 46 17.127835104   16.06 15.38     ~ 1381 1
22 SS 433 HXB 19 11 49.5647697480 +04 58 57.827127648   16.854 14.643     A7Ib 2253 4
23 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0
24 Min 1-92 pA* 19 36 18.9295687968 +29 32 49.785288144 12.13 12.35 11.75 11.54   B0.5IV[e] 267 0
25 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 2035 2
26 NGC 7009 PN 21 04 10.8155187648 -11 21 48.580157556   12.48 12.07     ~ 1020 1
27 V* R Aqr Sy* 23 43 49.4634303216 -15 17 04.176349872   8.823 7.683 9.37   M6.5-8.5e 823 0

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