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A new photometric study of T Tauri stars in the infrared
DOI: 10.1016/j.newast.2019.101286 Bibcode: 2020NewA...7401286C

Chen, P. S.; Liu, J. Y.; Shan, H. G.

We have compiled infrared photometric data from the literature of practically all T Tauri stars found up to date including 444 classical T Tauri stars (CTTSs), 1698 weak-line T Tauri stars (WTTSs) and 1258 not classified T Tauri stars (3400 in total) in addition to 196 post-T Tauri stars (PTTSs). From this data bank we extract the infrared charact…

2020 New Astronomy
AKARI 0
Infrared photometric study of SDSS selected narrow line Seyfert 1 galaxies
DOI: 10.1016/j.newast.2017.01.005 Bibcode: 2017NewA...54...30C

Chen, P. S.; Liu, J. Y.; Shan, H. G.

The infrared photometric study of SDSS selected Narrow Line Seyfert 1 Galaxies (NLS1s) is presented in this paper. We have made cross-identifications for such NLS1s with 2MASS and WISE observations. Finally 992 NLS1s have 2MASS and WISE counterparts. Comparisons of NLS1s with the Broad Line Seyfert 1 (BLS1s) and Seyfert 2 galaxies are made. It is …

2017 New Astronomy
AKARI 3
A new photometric study of Herbig Ae/Be stars in the infrared
DOI: 10.1016/j.newast.2015.09.001 Bibcode: 2016NewA...44....1C

Zhang, P.; Chen, P. S.; Shan, H. G.

In this paper we collected almost all HAeBe stars known so far (253 sources in total) to photometrically study their infrared properties. The 2MASS, WISE, IRAS and AKARI data are employed to make analyses. It is shown from several two-color diagrams that from 1 µm to 60 µm infrared radiations from circumstellar disks with the power law…

2016 New Astronomy
AKARI 30
Stellar contents and star formation in the young cluster Stock 18
DOI: 10.1016/j.newast.2011.07.015 Bibcode: 2012NewA...17..160B

Pandey, J. C.; Sagar, Ram; Bhatt, Himali

We have carried out deep (V ∼ 21 mag) UBVRI photometric study of the star cluster Stock 18. These along with archival Infrared data have been used to derive the basic cluster parameters and also to study the star formation processes in and around the cluster region. The distance to the cluster is derived as 2.8 ± 0.2 kpc while its age is estimated…

2012 New Astronomy
AKARI 4