Abstract
Data are presented on the first simultaneous X-ray and optical burst to
be measured in more than one optical color. Various analyses agree that,
to a first approximation, the optical burst is produced through
blackbody reprocessing of the X-ray burst, with a short delay. Depending
on the technique used, the value of the delay is 2 or 3 s. The smearing
of the optical signal is determined to be less than 3 s. The temperature
of the optical reprocessor ranges from approximately 25,000 K at
quiescence to approximately 50,000 K at burst maximum. An extinction
toward the source is derived from the color-color diagram, suggesting a
distance greater than or approximately equal to 2 kpc. The projected
effective area of the blackbody reprocessor is approximately 5 x 10 to
the 21st (D/5 kpc)-squared sq cm. The fraction of the total X-ray burst
energy converted into optical energy at all wavelengths is, within an
order of magnitude, approximately 3 percent. These parameters are
discussed in relation to the 4 hr orbital periodicity in the system
reported by Pedersen et al. (1981).
Original language | English |
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Pages (from-to) | 793-803 |
Journal | Astrophysical Journal |
Volume | 271 |
DOIs | |
Publication status | Published - 1 Aug 1983 |
Keywords / Materials (for Non-textual outputs)
- Ubv Spectra
- X Ray Sources
- Bursts
- Color-Color Diagram
- Colorimetry
- Optical Measurement