Fine X-Ray Tomography of Planetary Nebula

Details Fine X-Ray Tomography of Planetary Nebula Fine X-Ray Tomography of Planetary Nebula

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1147k&link_type=abstract

Chandra Proposal ID #04200847

Other

Chandra Proposal Id #04200847

Scientific paper

Although PNs have been thus made a stimulating new addition to the X-ray source populations, the X-ray emission mechanisms and the association between X-ray emitting regions and characteristic features observed in other wavelengths have not yet been clarified, and samples of X-ray PNs are still quite limited. To establish the nature of X-ray emitting PNs, observations with a finer spatial resolution are obviously inevitable. Here, to apply brand-new, X-ray-morphology diagnostic for another PNs with finer spatial resolution, and to verify the role of stellar wind which has been critical in the de facto standard model of the X-ray emission mechanism in PNs, we propose to observe the most promising candidate, NGC 4361 with Chandra ACIS-S.

Affiliated with

Also associated with

No associations

Rating

Fine X-Ray Tomography of Planetary Nebula 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 Fine X-Ray Tomography of Planetary Nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fine X-Ray Tomography of Planetary Nebula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1042346