Autoionizing Shocks along the Twisted Jets of NGC 4258

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We correlate new HIFI Fabry-Perot (FP) and KPNO Goldcam long-slit spectra with VLA radio, BIMA CO, and ROSAT X-ray datasets to study the twisted jets in this nearby Seyfert. The multi-arcminute extent of the jet and the extensive wavelength coverage of its interaction with the multiphase ISM make this jet an important laboratory for studying the processes likely to dominate the appearance of high-z radio galaxies. Our FP datacube covers the [OIII]lambda 5007 line at 60 km s(-1) FWHM resolution and shows that only the centermost, least twisted strand of the 3-strand Hα jet is prominent in high-excitation gas. Within 1 kpc radius this strand points N-S, coaligning with the radio jet, and is perpendicular to the subparsec nuclear disk delineated by water masers (Greenhill et al 1994 CfA preprint). It is thus, plausibly, the most recently active strand. The long-slit spectra span lambda lambda 3650--8950 Angstroms at 5 Angstroms resolution. Star motions mapped by the IR Ca triplet differ substantially from the mean gas velocities and line widths, arguing against virial broadening of the emission lines. In fact, emission-line ratios along the 5(') length of the line-emitting jets are consistent with those expected from shock excitation. After subtracting the starlight with the galaxy NGC 3115, we obtain sensitive limits on the N(+) , O(+) , and O(++) gas temperatures as well as useful upper limits on the important but undetected [NeIII] and HeII fluxes. These fluxes and limits, together with the gross kinematics, will be compared to the predictions of shock models. X-ray fluxes derived from the ROSAT PSPC and HRI datasets are consistent with jet emission from a Raymond-Smith thermal plasma with kT = 0.3 keV, logN_H ~ 20.0 cm(-2) , and luminosity 1.6*E(40) erg s(-1) . Gas can reach this temperature in a shock of velocity V_s~500 km s(-1) , a value consistent with the width and kinematic structure of the emission-line profiles. A modest disk gas density of 0.04 cm(-3) can produce the jet's x-ray flux. Hence, the shocked gas may be autoionized and entrained as the jets scrape along the molecular clouds that are known to be adjacent to the jets out to 2 kpc radius. This research is supported by NSF and NASA grants to UNC.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Autoionizing Shocks along the Twisted Jets of NGC 4258 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 Autoionizing Shocks along the Twisted Jets of NGC 4258, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Autoionizing Shocks along the Twisted Jets of NGC 4258 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1323370

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.