dc.contributor.author |
Lata, S. |
|
dc.contributor.author |
Pandey, A. K. |
|
dc.contributor.author |
Chen, W. P. |
|
dc.contributor.author |
Maheswar, G. |
|
dc.contributor.author |
Chauhan, N. |
|
dc.date.accessioned |
2015-05-06T05:21:10Z |
|
dc.date.available |
2015-05-06T05:21:10Z |
|
dc.date.issued |
2012 |
|
dc.identifier.uri |
http://hdl.handle.net/123456789/1061 |
|
dc.description.abstract |
We present results of multi-epoch (14 nights during 2007–2010) V-band photometry of the cluster NGC 1893 region to identify photometric variable stars in the cluster. The study identified a total of 53 stars showing photometric variability. The members associated with the region are identified on the basis of spectral energy distribution, J − H/H − K twocolour diagram and V/V − I colour–magnitude diagram. The ages and masses of the majority of pre-main-sequence sources are found to be ≤5Myr and in the range 0.5 ≤ M/M☉≤ 4, respectively. These pre-main-sequence sources hence could be T Tauri stars. We also determined the physical parameters like disc mass and accretion rate from the spectral energy distribution of these T Tauri stars. The periods of majority of the T Tauri stars range from 0.1 to 20 d. The brightness of Classical T Tauri stars is found to vary with larger amplitude in
comparison to weak line T Tauri stars. It is found that the amplitude decreases with increase in mass, which could be due to the dispersal of discs of massive stars. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
mn427-1449 |
|
dc.subject |
Stars: pre-main-sequence – stars: variables: T Tauri, Herbig Ae/Be – open clusters and associations: individual: NGC 1893. |
en_US |
dc.title |
Pre-main-sequence variable stars in young open cluster NGC 1893 |
en_US |
dc.type |
Article |
en_US |