PKS2152-69

Flux data

Available Data Downloads

Images, Maps, Spectra and SEDs

(definitions)Definitions.html
link to NED pagehttp://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=2152-69&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES

Infrared data

Radio data

Optical data

X-Ray data

1.4GHzPKS2152-69_files/r2152.zip
ESO Optical spectraPKS2152-69_files/s2152.zip


PKS2152-69

Optical spectrum taken with ESO telescopes.

Tadhunter et al. (1993)

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Wavelength/ Frequency Flux Units Reference 5GHz 12.65 Jy Morganti et al. (1993) [OIII] λ5007 -13.42 Log erg/cm2/s Tadhunter et al. (1993) http://adsabs.harvard.edu/abs/1993MNRAS.263.1023Mhttp://adsabs.harvard.edu/abs/1993MNRAS.263..999Tshapeimage_15_link_0shapeimage_15_link_1

Other name:

Redshift:

RA (j2000):

Dec (j2000):

Optical class:

Radio Class:

0.027

21 57 06.0

-69 41 24

BLRG

FRI/FRII

-

PKS2152-69

K-band (2.2 microns) image. 2x2 arcmins.

Inskip et al. (2010)


N

E

N

E

UK Schmidt image, λ4680A, width 4 arcmins.

ISAAC K-band dataPKS2152-69_files/out_2152.fits

Notes

    The optical spectrum of this radio galaxy shows a  moderate-ionization emission line spectrum along with broad wings to the Balmer lines. The continuum spectrum is typical of early type galaxies. The object has a bright emission line blob ~10 arcsec to the NE of the nucleus that shows an unusually high ionization state (see Tadhunter et al. 1987, 1988).

    At radio wavelengths PKS2152-69 shows hybrid FRI/FRII characteristics, and the NE emission line blob is found to be situated close to a knot in the radio jet, suggesting that a jet-cloud interaction has taken place at this location (Fosbury et al. 1998, MNRAS,  296, 701).