Abstract

view Abstract Citations (46) References (32) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The LkH alpha 101 Infrared Cluster Barsony, M. ; Schombert, J. M. ; Kis-Halas, K. Abstract IRIM on the KPNO 1.3-m telescope is used to map an 8-ft x 12-ft area, corresponding to a 1.9- x 2.8-pc field centered on the Herbig Ae/Be star, LkH-alpha 101, in the near-infrared J and K bandpasses. The discovery of an embedded cluster of more than 100 young stellar objects within this area is reported. The present completeness limits are estimated at 16.5 mag at J and 14.5 mag at K. Four types of cluster members, defined by their location in the K versus J-K color magnitude diagram, are identified. The embedded cluster population of the LkH-alpha 101 cloud core is found to consist of 16 Class I sources, 39 probable Class I sources, 40 young embedded low-mass PMS stars, and 46 young, embedded brown dwarf candidates. From the relative numbers of sources of each type, an upper limit for the accreting protostar phase of 400,000 yr is estimated. The spatial distribution of the sources in the cloud core is highly nonuniform, such that the youngest sources are the most centrally concentrated. Publication: The Astrophysical Journal Pub Date: September 1991 DOI: 10.1086/170496 Bibcode: 1991ApJ...379..221B Keywords: B Stars; Brown Dwarf Stars; Infrared Sources (Astronomy); Open Clusters; Pre-Main Sequence Stars; Star Formation; Color-Magnitude Diagram; Deep Space; Near Infrared Radiation; Protostars; Sky Surveys (Astronomy); Spatial Distribution; Star Distribution; Astrophysics; CLUSTERS: OPEN; INFRARED: SOURCES; STARS: BE; STARS: BROWN DWARFS; STARS: INDIVIDUAL ALPHANUMERIC: LKH ALPHA 101; STARS: PRE--MAIN-SEQUENCE full text sources ADS | data products SIMBAD (3)

Full Text
Paper version not known

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 call

Disclaimer: 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.