Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.336..736c&link_type=abstract
Monthly Notice of the Royal Astronomical Society, Volume 336, Issue 3, pp. 736-746.
Astronomy and Astrophysics
Astronomy
8
Stars: Formation, Hii Regions, Ism: Structure, Infrared: Ism, Infrared: Stars, Radio Continuum: Ism
Scientific paper
We report on a multi-wavelength study of images in the mid-infrared (MIR), Hα and radio continuum of an unusual HII region, G308.70 + 0.60. Using images from the Midcourse Space Experiment (MSX) between 8.3 and 21.3 μm, from the AAO/UK Schmidt Telescope (UKST) deep, high-resolution, Hα survey of the plane, and from the Molonglo Observatory Synthesis Telescope (MOST) Galactic plane survey in the radio continuum at 843 MHz, we have investigated the morphology of the nebula and propose that there is an interaction between the interstellar medium and a star lying inside the large nebular bubble. Secondary star formation appears to have occurred in several places on the dense rim of the bubble. In one such site, this has resulted in a luminous MIR double star, situated within the rim of the nebular ring, that has created its own local bubble.
Cannon Russell D.
Cohen Martin
Green Anne J.
Mader Stacy
Parker Quentin A.
No associations
LandOfFree
Mid-infrared, Hα and radio continuum images of an unusual HII region, G308.70 + 0.60 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 Mid-infrared, Hα and radio continuum images of an unusual HII region, G308.70 + 0.60, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mid-infrared, Hα and radio continuum images of an unusual HII region, G308.70 + 0.60 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-950502