Observe Bright Atol Sources at High Mass Accretion Rates

Details Observe Bright Atol Sources at High Mass Accretion Rates Observe Bright Atol Sources at High Mass Accretion Rates

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2935c&link_type=abstract

Chandra proposal ID #11400037

Physics

Scientific paper

GX 13+1 has some history of line absorption in the Fe K region with XMM and Chandra. We want to confirm the existence of blue-shifted absorption, detect line flux and shift variability possibly in correlation with its spectral (banana) branch and source luminosity, as well as verify and investigate some unusual line detections ( i.e. Cr XXIV, Mn XXV). We employ a strategy of 5 x ~30 ks observations scattered over longer time spans with the goal to cover as much of the banana branch as possible. The ~30 ks length of each observation guarantees the same detection significance as in the existing observation.

Affiliated with

Also associated with

No associations

Rating

Observe Bright Atol Sources at High Mass Accretion Rates 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 Observe Bright Atol Sources at High Mass Accretion Rates, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observe Bright Atol Sources at High Mass Accretion Rates will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-838936