74 research outputs found
Wavelet-based cross-correlation analysis of structure scaling in turbulent clouds
We propose a statistical tool to compare the scaling behaviour of turbulence
in pairs of molecular cloud maps. Using artificial maps with well defined
spatial properties, we calibrate the method and test its limitations to
ultimately apply it to a set of observed maps. We develop the wavelet-based
weighted cross-correlation (WWCC) method to study the relative contribution of
structures of different sizes and their degree of correlation in two maps as a
function of spatial scale, and the mutual displacement of structures in the
molecular cloud maps. We test the WWCC for circular structures having a single
prominent scale and fractal structures showing a self-similar behavior without
prominent scales. Observational noise and a finite map size limit the scales
where the cross-correlation coefficients and displacement vectors can be
reliably measured. For fractal maps containing many structures on all scales,
the limitation from the observational noise is negligible for signal-to-noise
ratios >5. (abbrev). Application of the WWCC to the observed line maps of the
giant molecular cloud G333 allows to add specific scale information to the
results obtained earlier using the principle component analysis. It confirms
the chemical and excitation similarity of CO and CO on all
scales, but shows a deviation of HCN at scales of up to 7' (~7 pc). This can be
interpreted as a chemical transition scale. The largest structures also show a
systematic offset along the filament, probably due to a large-scale density
gradient. The WWCC can compare correlated structures in different maps of
molecular clouds identifying scales that represent structural changes such as
chemical and phase transitions and prominent or enhanced dimensions.Comment: 26 pages, 41 figures, accepted to A&
Understanding the relationship between the environment of the black hole and the radio jet: optical spectroscopy of compact AGN
We aim to investigate the relationship between radio jet activity on
parsec-scales and the characteristics of both the bright active galactic nuclei
(AGN) and their broad line regions (BLR). For this purpose, we combine 2cm Very
Long Baseline Array observations of AGN with their optical spectral
observations. This would enable us to investigate the optical spectra of a set
of 172 relativistically beamed, flat-spectrum AGN with the nuclear disk
oriented near to the plane of sky. Here, we present first results from optical
spectroscopic observations of the brightest AGN from the 2 cm VLBA survey, and
show a diversity of their spectral morphologies.Comment: 2 pages, to be published in the Proceedings of "Multiwavelength AGN
Surveys", Cozumel, Dec 8 - 12, 200
On the jet speeds of classical double radio sources
A simple integral relation is obtained for the distribution functions of jet
speeds and jet-counterjet flux asymmetries of classical double radio sources.
Analytic expressions relating the mean jet speed and the mean jet flux
asymmetry, and their variances are derived. The results are considered in the
light of orientation-based unified schemes, and an analytical equation for the
critical angle separating quasars and radio galaxies is derived. The mean jet
speeds of classical double radio sources are estimated using the asymmetry of
jet-counterjet flux densities taken from the 3CRR and B2 samples. For FRI radio
sources the mean jet speed is ~0.54c (with a standard error SE=0.03c), while
for FRII low-redshift radio galaxies and intermediate redshift quasars the
values found are ~0.4c (SE=0.06c) and >0.6c respectively.Comment: 7 pages, 2 figures. The revised version is accepted for publication
in the MNRA
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