Description
This star was originally a small blue sun of a star class of critical interest to the Triglavian Collective. Manipulation of this star by a Triglavian Dazh Porevitium Transmuter has caused profound changes in this stellar body, and throughout the system surrounding it.
More typical members of this star class of relatively common dwarf stars are often planet-bearing or accompanied by planetary dust clouds. Many stars of this kind rotate quickly and the class is known for strong hydrogen and ionized metal lines in stellar spectroscopy.
