2009MNRAS.394..533G


Query : 2009MNRAS.394..533G

2009MNRAS.394..533G - Mon. Not. R. Astron. Soc., 394, 533-546 (2009/March-3)

Are red 2MASS QSOs young?

GEORGAKAKIS A., CLEMENTS D.L., BENDO G., ROWAN-ROBINSON M., NANDRA K. and BROTHERTON M.S.

Abstract (from CDS):

We use photometric data from the Spitzer mission to explore the mid- and far-infrared properties of 10 red QSOs (J - K > 2, R - K > 5mag) selected by combining the Two Micron All Sky Survey (2MASS) in the near-infrared with the Sloan Digital Sky Survey (SDSS) at optical wavelengths. Optical and/or near-infrared spectra are available for 8/10 sources. Modelling the spectral energy distribution (SED) from ultraviolet to far-infrared shows that moderate dust reddening (AV= 1.3-3.2) can explain the red optical and near-IR colours of the sources in the sample. There is also evidence that red QSOs have 60/12µm luminosity ratio higher than PG QSOs (97 per cent significance). This can be interpreted as a higher level of star formation in these systems (measured by the 60-µm luminosity) for a given active galactic nucleus (AGN) power (approximated by the 12-µm luminosity). This is consistent with a picture where red QSOs represent an early phase of AGN evolution, when the supermassive black hole is enshrouded in dust and gas clouds, which will eventually be blown out (possibly by AGN driven outflows) and the system will appear as typical optically luminous QSO. There is also tentative evidence significant at the 96 per cent level that red 2MASS QSOs are more often associated with radio emission than optically selected SDSS QSOs. This may indicate outflows, also consistent with the young AGN interpretation. We also estimate the space density of red QSOs relative to optically selected SDSS QSOs, taking into account the effect of dust extinction and the intrinsic luminosity of the sources. We estimate that the fraction of red QSOs in the overall population increases from 3 per cent at MK= -27.5mag to 12 per cent at MK = -29.5mag. This suggests that reddened QSOs become more important at the bright end of the luminosity function. If red QSOs are transition objects on the way to becoming typical optically luminous QSOs, the low fractions above suggest that these systems spent less than 12 per cent of their lifetime at the `reddened' stage.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): surveys - galaxies: active - quasars: general - infrared: general

Simbad objects: 17

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Number of rows : 17
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 HD 166 BY* 00 06 36.7840068588 +29 01 17.412693890   6.82 6.07 5.6   G8V 392 0
2 IRAS F00344-0130 Sy1 00 36 59.8312535184 -01 13 32.518899516   21.63 20.76 20.023 18.630 ~ 15 0
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
4 QSO B0132-097 QSO 01 34 35.6657627616 -09 31 02.903742300   24.52 22.70 20.80   ~ 113 2
5 2MASS J08250205+4716519 Sy1 08 25 02.059 +47 16 51.99   21.19 20.77 20.45   ~ 17 0
6 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
7 2MASS J12521292+0715046 QSO 12 52 12.9225099924 +07 15 04.710477778           ~ 2 0
8 * 61 Vir PM* 13 18 24.3139864471 -18 18 40.297748582 5.710 5.440 4.740     G6.5V 742 1
9 2MASS J13212289+4502248 AG? 13 21 22.89 +45 02 24.8           ~ 1 0
10 NVSS J134039+051420 rG 13 40 39.6742932379 +05 14 19.620123278   20.14 19.45 18.99   ~ 7 0
11 BD+28 2411 PM* 15 12 45.9225885960 +27 55 14.046577500   9.97 9.24     G0 28 0
12 2MASS J15333418+0735056 AG? 15 33 34.18 +07 35 05.7           ~ 2 0
13 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
14 BD+33 2642 pA* 15 51 59.8854348048 +32 56 54.329485272 9.806 10.61 10.73 10.884 10.961 O7p 456 0
15 2MASS J17042115+2433409 AG? 17 04 21.1504290648 +24 33 40.911185592           ~ 1 0
16 IRAS F20460-0035 QSO 20 48 37.2525289848 -00 24 37.189819620           ~ 8 0
17 2MASS J20562975-0650553 AG? 20 56 29.7555331200 -06 50 55.342170348           ~ 2 0

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