Abstract
Statistical analysis of a young stellar cluster surrounding the source IRAS 05137+3919 at a distance of 4.4 kpc reveals four binary objects and one triplet. These include a pair of Ae/Be Herbig stars. The percent content of multiple systems in the cluster is mf = 5-6% and cp = 10-13%. The masses of the components of the multiple systems range from ~1 to 8 M ⨀ and logP (P is the rotation period in years) ranges from 4.4 to 4.7. The median value of the mass ratio of the components is q = 0.86. The percentage and parameters of the multiple systems are similar to data on other star formation regions (ONC, Perseus, UScoA) for which the parameters mf and cp are comparable to the results obtained for the stellar population of the field.
Sign-in/Register to access full text options 
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.
