THE STRUCTURE OF THE ACCRETION DISK IN THE ACCRETION DISK CORONA X-RAY BINARY 4U 1822-371 AT OPTICAL AND ULTRAVIOLET WAVELENGTHS

Journal Article · Wed Jan 20 04:00:00 EST 2010 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/709/1/251· OSTI ID:21392359

Bayless, Amanda J; Robinson, Edward L; Cornell, Mark E ^[1]; Hynes, Robert I ^[2]; Ashcraft, Teresa A ^[3]

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1. Department of Astronomy, University of Texas at Austin, 1 University Station, Austin, TX 78712-0259 (United States)
2. Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803 (United States)
3. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287-1404 (United States)

The eclipsing low-mass X-ray binary 4U 1822-371 is the prototypical accretion disk corona (ADC) system. We have obtained new time-resolved UV spectroscopy of 4U 1822-371 with the Advanced Camera for Surveys/Solar Blind Channel on the Hubble Space Telescope and new V- and J-band photometry with the 1.3 m SMARTS telescope at Cerro Tololo Inter-American Observatory. We use the new data to construct its UV/optical spectral energy distribution and its orbital light curve in the UV, V, and J bands. We derive an improved ephemeris for the optical eclipses and confirm that the orbital period is changing rapidly, indicating extremely high rates of mass flow in the system, and we show that the accretion disk in the system has a strong wind with projected velocities up to 4000 km s{sup -1}. We show that the disk has a vertically extended, optically thick component at optical wavelengths. This component extends almost to the edge of the disk and has a height equal to approx0.5 of the disk radius. As it has a low brightness temperature, we identify it as the optically thick base of a disk wind, not as the optical counterpart of the ADC. Like previous models of 4U 1822-371, ours needs a tall obscuring wall near the edge of the accretion disk, but we interpret the wall as a layer of cooler material at the base of the disk wind, not as a tall, luminous disk rim.

• OSTI ID: 21392359
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 709; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ACCRETION DISKS
ANALOG-TO-DIGITAL CONVERTERS
BRIGHTNESS
CAMERAS
COSMIC RADIO SOURCES
ECLIPSE
ELECTROMAGNETIC RADIATION
ELECTRONIC EQUIPMENT
ENERGY SPECTRA
EQUIPMENT
IONIZING RADIATIONS
MASS
OPTICAL PROPERTIES
PHOTOMETRY
PHYSICAL PROPERTIES
PULSARS
RADIATIONS
RESOLUTION
SPECTRA
TELESCOPES
TIME RESOLUTION
TIMING PROPERTIES
ULTRAVIOLET RADIATION
WAVELENGTHS
X RADIATION