High-Velocity Gas in the Luminous H II Regions of NGC 1530

Details High-Velocity Gas in the Luminous H II Regions of NGC 1530 High-Velocity Gas in the Luminous H II Regions of NGC 1530

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12..252r&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Galaxies: Abundances, H Ii Regions

Scientific paper

We are carrying out a systematic study of the ensuremath {{H}alpha } emission line profiles from the H II regions in NGC 1530 (Knapen et al. 2001) based on a data cube from the TAURUS Fabry-Perot scanner, on the 4.2m WHT, La Palma. The data are of high S:N ratio, high spatial resolution (seeing ~ 0.6 arcsec ) and velocity resolution, FWHM, of 18 kms ensuremath {^{-1}} . The observations reveal, from the luminous regions, high velocity components forming low intensity wings to the intense emission peak. We cannot tell whether they are absent in the less luminous regions, or below the noise level. We detected similar high velocity features from M100, NGC 3359, and NGC 6951 (see e.g., Rozas et al. 1998).

Affiliated with

Also associated with

No associations

Rating

High-Velocity Gas in the Luminous H II Regions of NGC 1530 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 High-Velocity Gas in the Luminous H II Regions of NGC 1530, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-Velocity Gas in the Luminous H II Regions of NGC 1530 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1043519