1 / 4

New Analysis of Open Clusters Using CCD Photometry

New Analysis of Open Clusters Using CCD Photometry. Kayla Young. Future Studies. Add more Open Clusters to compare more ages and absolute magnitude. Using a CCD Imager and B and V filters take images of clusters, instead of downloading them.

infinity
Download Presentation

New Analysis of Open Clusters Using CCD Photometry

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. New Analysis of Open Clusters Using CCD Photometry Kayla Young

  2. Future Studies • Add more Open Clusters to compare more ages and absolute magnitude. • Using a CCD Imager and B and V filters take images of clusters, instead of downloading them. • Use better software, to get a deeper analysis of a cluster.

  3. Conclusion • The data supported the initial null hypothesis that the age of the open clusters are directly correlated with the absolute magnitude. This was proven because the youngest cluster NGC 1094 had the strongest absolute magnitude and the oldest cluster NGC 104 had the weakest absolute magnitude.

  4. Discussion • Many of the absolute magnitudes in the cluster NGC 104 were extremely weak, and many of the absolute magnitude sin the cluster NGC 6694 were very strong.

More Related