Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002chjaa...2..501z&link_type=abstract
Chinese Journal of Astronomy & Astrophysics, Vol. 2, p. 501-524
Astronomy and Astrophysics
Astrophysics
17
Galaxies: Active, Galaxies: Seyfert, Radiation: Continuum
Scientific paper
We have performed a statistical study of the properties of the broad band continuum of Narrow Line Seyfert 1 galaxies (NLS1s) by collecting ratio, infrared, optical and X-ray continuum data from various databases and compared the results with control samples of Broad Line Seyfert 1 galaxies (BLS1s). We find that the fraction (˜ 6%) of Radio Loud (RL) NLS1s is significantly less than that of BLS1s (˜ 13%), which is caused by the lack of radio-very-loud sources in the former. The rarity of RL NLS1s, especially radio-very-loud ones, is consistent with the scenario of small black hole and high accretion rate for NLS1s. Six new radio loud NLS1s are found and five RL NLS1 candidates are presented. In comparison with the BLS1s, the NLS1s tend to have stronger far infrared emission, cooler infrared colors and redder B-K color, which suggests that NLS1s are hosted by dust-richer nuclei. The NLS1s also show steeper soft X-ray spectrum and large soft X-ray to optical flux ratio, while a significant fraction show flat soft X-ray spectra. At least two factors can account for this, absorption and spectral variability. We also perform a correlation analysis between various broad band data. It is found that most correlations identified for NLS1s are also valid for radio quiet BLS1s: (1) the optical colors are anti-correlated with X-ray spectral index; (2) higher optical, X-ray and NIR luminosity objects show bluer optical colors and red H-K color; (3) higher luminosity objects show warmer IRAS color; (4) the radio loudness correlates with B-K and X-ray to optical flux ratio. Radio loud objects behave somewhat differently in a few correlations.
Wang Ting-Gui
Zhou Hong-Yan
No associations
LandOfFree
Properties of Broad Band Continuum of Narrow Line Seyfert 1 Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Properties of Broad Band Continuum of Narrow Line Seyfert 1 Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of Broad Band Continuum of Narrow Line Seyfert 1 Galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-962910