J/ApJ/625/78 QSOs properties (Hao+, 2005)
The physical connections among infrared QSOs, Palomar-Green QSOs, and
narrow-line Seyfert 1 galaxies.
Hao C.N., Xia X.Y., Mao S., Wu H., Deng Z.G.
<Astrophys. J., 625, 78-88 (2005)>
=2005ApJ...625...78H 2005ApJ...625...78H (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei ; QSOs
Keywords: galaxies: active - galaxies: evolution - galaxies: interactions -
galaxies: ISM - galaxies: starburst - quasars: general
Abstract:
We study the properties of infrared-selected QSOs (IR QSOs), optically
selected Palomar-Green QSOs (PG QSOs), and narrow-line Seyfert 1
galaxies (NLS1s). We compare their properties from the IR to the
optical and examine various correlations among the black hole mass,
accretion rate, star formation rate, and optical and IR luminosities.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 78 110 Various physical parameters
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See also:
II/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989)
II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986)
J/MNRAS/308/897 : QDOT all-sky IRAS redshift survey (Lawrence+, 1999)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 7 A7 --- Type Object type (1)
9- 20 A12 --- Name Object name (2)
22- 26 F5.3 --- z Redshift
28- 32 F5.3 [solMass] logM Log of the Blackhole mass
34- 39 F6.3 [solLum] logLIR Log of the IR luminosity
41 A1 --- l_logLIR [a] Upper limti flag on logLIR (3)
43- 48 F6.3 [solLum] logLopt Log of the optical luminosity (4)
50- 55 F6.3 [solLum] logLBol Log of the Bolometric luminosity (5)
57- 62 F6.3 --- logLEdd Log of the Eddington luminosity ratio
64- 69 F6.3 [solLum] logL60um ? Log of the 60µm monochromatic
luminosity
71 A1 --- l_logL60um [b] Upper limit flag on logL60um
73- 78 F6.3 [solLum] logLHB ? Log of the Hβ luminosity
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Note (1): Object type defined as follows:
IR QSOs = Infrared QSOs
NLS1s = Narrow-line Seyfert 1 galaxies
PG QSOs = Palomar-Green QSOs
Note (2): For IRAS names, IRHHMMm+DDMM stands for IRAS HHMMm+DDMM, and
FHHMMm+DDMM stands for IRAS FHHMMm+DDMM.
Note (3): A "a" indicates the flux density in at least one IRAS band is an upper
limit for objects whose infrared properties were taken from IRAS; the
infrared luminosity in at least one band is an upper limit for objects
from Table 2 of Haas et al. (2003A&A...402...87H 2003A&A...402...87H).
Note (4): Monochromatic luminosity at 5100Å, λ Lλ(5100Å).
Note (5): Bolometric luminosity of AGN (9λ Lλ(5100Å)).
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History:
From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 23-Nov-2005