Variability type of MisV1147			Seiichi Yoshida

Referring to:

  GCVS Variability Types and Distribution Statistics of Designated
  Variable Stars According to their Types of Variability
  http://www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/vartype.txt

a young stellar object can be classified one of the following types:

  I, IA, IB, IN, INA, INB, IS, ISA, ISB, INS, INSA, INSB, IT, INT, INST

1) Irregular variation

   First of all, "I" is attached because the variation is irregular.

2) Spectral class

   When the spectral class is between O-A, "A" is attached. 

   When the spectral class is between F-M, "B" is attached. However,
   when the star is classified into 5) T Tauri type, "T" is attached
   instead of "B".

3) Nebulae

   When nebulae are found around the star, "N" is attached.

4) Rapid variation

   When the star shows about 0.5 or 1.0 mag variation in short time,
   within several hours or days, "S" is attached.

5) T Tauri type

   When the spectral class is between F-M, and the emission lines of
   Fe II at 4046/4132 angstrom and the absorption line of Li at 6707
   angstrom are visible, "T" is attached.

In the case of MisV1147, no nebula is found, so "N" is not attached. 
It shows the rapid variation, so "S" is attached. 

Therefore, the variability type of MisV1147 will be one of ISA, ISB or
IST.