This program monitors the stability of the constant terms in the NUV dispersion solutions. To monitor for any changes comma the program observes HD 6655 at selected cenwaves for the three NUV grating
The Spiral Planetary Nebula (NGC 5189), exhibits spectacular pointsymmetricmorphology indicative of a number of collimated outflows. The WO1 central starhas lost its hydrogenrich envelope, possibly th
Outbursts of super-massive black holes openParSMBHsclosePar have a significant impact on structure formation and evolution. However comma AGN heating from SMBHs has not been well studied in galaxy gr
