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| Query : 1994A&A...286..497P |
1994A&A...286..497P - Astronomy and Astrophysics, volume 286497-500 (1994/6-2)
Hercules X-1 pulse profile simulation.
PANCHENKO I.E. and POSTNOV K.A.
Abstract (from CDS):
We performed calculations of the average X-ray pulse profile observed from the X-ray pulsar Hercules X-1 at the "main-on" state of the 35-day cycle. We assume that accretion in this source takes place in three distinct zones on the neutron star surface: two magnetic poles and a circle-like area around the pole with lower magnetic field strength, which is connected with a complex (presumably quadrupole) structure of the neutron star magnetic field at its surface.
Abstract Copyright: ∼
Journal keyword(s): stars: neutron - pulsars: individual: Her X-1
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | V* HZ Her | LXB | 16 57 49.8110126616 | +35 20 32.486555472 | 11.90 | 14.89 | 13.63 | 13.88 | B3/6ep | 2172 | 0 | |
| 2 | V* V2246 Cyg | HXB | 20 32 15.2749858128 | +37 38 14.843024844 | 22.16 | 19.41 | 17.32 | 15.18 | B0Ve | 480 | 0 |
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