Volume 11, Issue 3 (2-2011)                   2011, 11(3): 187-196 | Back to browse issues page

XML Persian Abstract Print


Download citation:
BibTeX | RIS | EndNote | Medlars | ProCite | Reference Manager | RefWorks
Send citation to:

N F, MT M. Photometry of Central Parts of M33 Galaxy in Near Infrared. Journal title 2011; 11 (3) :187-196
URL: http://jsci.khu.ac.ir/article-1-1462-en.html
Abstract:   (5450 Views)
In this paper, we analyze, near infra red images of the central region of the local group galaxy M33.  These images were obtained in K band with the UFTI instrument, installed on the UKIRT telescope. This is a part of a bigger project started in 2003 with an aim to investigate RGB and AGB stars in M33. K band magnitude was obtained for 18509 stars by fitting appropriate PSF models to stellar profiles in the images. ‎The ‎final ‎catalogue ‎was ‎obtained ‎by ‎ calibrating ‎instrumental ‎magnitude ‎to ‎standard‎ ‎system.‎ Cross correlation methods was manipulated to assign J-K color index to each star. A color magnitude diagram was plotted which represents population of RGB, AGB and Carbon stars  in the core of M33 galaxy
Full-Text [PDF 351 kb]   (1560 Downloads)    
Type of Study: S |
Published: 2011/02/15

Add your comments about this article : Your username or Email:
CAPTCHA

Send email to the article author


Rights and permissions
Creative Commons License This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.

© 2024 CC BY-NC 4.0 | Quarterly Journal of Science Kharazmi University

Designed & Developed by : Yektaweb