Details on Acronym: MPE | |
MPE | (Max Planck inst. fur Extraterrestriche physik) |
Write: | <<MPE +x.x+yy.y>> |
N: | 22 |
Object: | * (SIMBAD class: Star) |
Stat: | is completely incorporated in Simbad |
in source: | NAME Gal Center |
Ref: | =1995ApJ...445L..23E |
by | ECKART A. , GENZEL R., HOFMANN R., SAMS B.J., TACCONI-GARMAN L.E. |
Astrophys. J., 445, 23-26 (1995) | |
High angular resolution spectroscopic and polarimetric imaging of the Galactic Center in the near-infrared. | |
o | <MPE +x.x+yy.y> N=2. |
Ref: | =1995ApJ...447L..95K |
by | KRABBE A. , GENZEL R., ECKART A., NAJARRO F., LUTZ D., CAMERON M., KROKER H., TACCONI-GARMAN L.E., THATTE N., WEITZEL L., DRAPATZ S., GEBALLE T., STERNBERG A., KUDRITZKI R. |
Astrophys. J., 447, 95-99 (1995) | |
The nuclear cluster of the Milky Way: star formation and velocity dispersion in the central 0.5 parsec. | |
o | Table 1: <MPE +x.x+yy.y> N=10, <NAME AF NW> |
Ref: | =1999ApJ...523..248O |
by | OTT T. , ECKART A., GENZEL R. |
Astrophys. J., 523, 248-264 (1999) | |
Variable and embedded stars in the galactic center. | |
o | Table 2: <[OEG99] NNN> (Nos 1-218). Table 2: <GCIRS NNWW> N=7 new. Table 2: <MPE +x.x+yy.y> N=10 new. |
Origin | of the Acronym: L (1996ApJ...470..864B) |