Orion OB1


Orion OB1 is a contingent group of several dozen hot giant stars of spectral types O and B in Orion. Associated are thousands of lower-mass stars, and a number of protostars. It is part of the larger Orion [molecular cloud complex]. Owing to its relative closeness and complexity it is the most closely studied OB association.
The Orion OB1 consists of the following subgroups:
Signatures of stellar debris disk evolution have been detected in the 1a and 1b subgroups.