[vsnet-campaign-xray 351] SWIFT J1753.5-0127: Swift UVOT

[Makoto Uemura]

SWIFT J1753.5-0127: Swift UVOT

    ATel #553 shows multiband photometry of the new X-ray 
transient with Swift UVOT.  According to the report, it has B-V~0, 
which is typical for the thermal emisison from multicolor accretion 
disks in black hole X-ray binaries.  They also report that no 
rapid variation (10-1000s) was detected.

For more detailed information, see:
ATel#553:  http://www.astronomerstelegram.org/?read=553

Regards,
Makoto Uemura
Hiroshima University