klamppauksella

Klampauschella is a type of ultracompact H II region galaxy. It is characterized by its small size and high surface brightness, making it an ideal subject for astrophysical study.

Located approximately 45 million light-years away in the constellation Cassiopeia, Klampauschella is a relatively small galaxy, measuring only 350 parsecs in diameter. Despite its compact size, it contains a high mass of around 10^5 solar masses. This is in contrast to typical H II region galaxies, which are often found with sizes ranging from 100 to 1000 parsecs.

The galaxy is named after the astronomer Pete Klamp, who first observed the object in the 1970s. The choice of name is in accordance with standard nomenclature for nova-like variables, though in this instance, Klampauschella has been found not to have the same variability characteristics as most other objects with this classification.

Studies have shown that the galaxy exhibits unique properties when compared to other H II regions. Its implied lifetime in the dense gas phase, derived from models simulating photoionization and grain accretion effects, is on the order of 1/5 that of certain H II region objects, indicating intrinsically shorter internal relaxation timescales.

Continued study of Klampauschella's spectral and temporal properties may reveal further insights into the galactic evolutionary processes underlying its nongalactic and less alphabetical denotations.