Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525)

Details Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525) Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525)

2008-08-15

arxiv.org/abs/0808.2139v1

Astronomy and Astrophysics

Astrophysics

Accepted for publication in MNRAS

Scientific paper

10.1111/j.1745-3933.2008.00545.x

In the microquasar V4641 Sgr the spin of the black hole is thought to be misaligned with the binary orbital axis. The accretion disc aligns with the black hole spin by the Lense-Thirring effect near to the black hole and further out becomes aligned with the binary orbital axis. The inclination of the radio jets and the Fe$K\alpha$ line profile have both been used to determine the inclination of the inner accretion disc but the measurements are inconsistent. Using a steady state analytical warped disc model for V4641 Sgr we find that the inner disc region is flat and aligned with the black hole up to about $900 R_{\rm g}$. Thus if both the radio jet and fluorescent emission originates in the same inner region then the measurements of the inner disc inclination should be the same.

Affiliated with

Also associated with

No associations

Rating

Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525) 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 Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-651316