Soft X-Ray Diagnostics of a Possible ADC in X2127+119

Details Soft X-Ray Diagnostics of a Possible ADC in X2127+119 Soft X-Ray Diagnostics of a Possible ADC in X2127+119

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..102w&link_type=abstract

Chandra Proposal ID #01400360

Physics

Chandra Proposal Id #01400360

Scientific paper

X2127+119 exhibits dips with a period of 17.1 hours. Its accretion disk may possess an ionized corona (ADC), though the apparent lack of reprocessing of a bright type I burst disputes this possibility. One diagnostic of ADC conditions is strong discrete emission, whose analysis sheds light upon the location of and temperature and ionization level in the reprocessing gas. To date this system has never been observed spectroscopically with good energy resolution or at soft X-ray energies (where spectral features abound). We propose two observations of X2127+119: one using the ACIS-S-LETG and one using the ACIS-S-HETG. We show that X2127+119 is sufficiently bright to produce good spectra and that such spectra will likely include numerous strong soft emission features.

Affiliated with

Also associated with

No associations

Rating

Soft X-Ray Diagnostics of a Possible ADC in X2127+119 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 Soft X-Ray Diagnostics of a Possible ADC in X2127+119, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Soft X-Ray Diagnostics of a Possible ADC in X2127+119 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1553542