Checking 206 Stardial-images from 1996 to 2000 showed
IRAS 19045-0414 to be a Mira star.
The period is about 300 days and the amplitude greater
than 2 mag in I.
The star is too faint to be measured on the stardial-images
with MIRA, but there are clear Maxima around 2450700,
2451000 and 2450310.
A check of the available TASS-measurements
proofed the star (TASS J190711.5-041004)
to be variable and the Maxima around 50700
and 51000.
The USNO-A2.0 gives R=13.9 and B=17.6 for this star
(0825-14497900).
The Stardial-project is one of the most fascinating aspects of the WEB,
many thanks to Peter McCullough!!
The TASS-Database
is a very valuable source to check and verify new
findings. Many thanks to the TASS