| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1779115 | New Astronomy | 2013 | 9 Pages |
Abstract
⺠Support in favour of triggered star formation towards the direction of the two nebulae located at the periphery of the cluster. ⺠The fraction of disk bearing stars increases towards the periphery of the cluster. ⺠Evidence in support of the notion that the mechanisms for disk dispersal operate less efficiently for low-mass stars. ⺠Our result for this region support the claim that the CTTSs and WTTSs are coeval and have indistinguishable properties.
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Authors
A.K. Pandey, M.R. Samal, N. Chauhan, C. Eswaraiah, J.C. Pandey, W.P. Chen, D.K. Ojha,