Abstract
The results of a spectroscopic investigation of four stars comprising a Trapezium system in the nebula Sh 155 are presented. The stars have a number of emission lines typical of red emission stars and T Tau stars. This system is one of the 13 systems which we have found in the Palomar atlas. It is shown that all of these systems are members of OB associations.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
