• Search Research Projects
  • Search Researchers
  • How to Use
  1. Back to previous page

Observational study of the relation between the AGB evolution and the space distribution of AGB stars

Research Project

Project/Area Number 08640338
Research Category

Grant-in-Aid for Scientific Research (C)

Allocation TypeSingle-year Grants
Section一般
Research Field Astronomy
Research InstitutionNational Astronomical Observatory

Principal Investigator

NOGUCHI Kunio  National Astronomical Observatory, Division of Optical and Infrared Astronomy, Associate Professor, 光学赤外線天文学・観測システム研究系, 助教授 (10111824)

Project Period (FY) 1996 – 1997
Project Status Completed (Fiscal Year 1997)
Budget Amount *help
¥2,200,000 (Direct Cost: ¥2,200,000)
Fiscal Year 1997: ¥900,000 (Direct Cost: ¥900,000)
Fiscal Year 1996: ¥1,300,000 (Direct Cost: ¥1,300,000)
KeywordsEvolution of AGB stars / Carbon stars / M-type stars / Distribution of AGB stars
Research Abstract

We have investigated the evolution of asymptotic giant branch (AGB) stars on the basis of the space distribution of AGB stars. There are two kinds of AGB stars : Carbon stars and M-type stars. We suspect that the space distributions of these two-types of stars are different from each other and that the evolutionary sequence of AGB stars is not the same in the whole Galaxy. To clarify the difference or the similarity of the evolutionary sequence depending on the location in the Galaxy, it is essential to know the space distribution of carbon stars and M-type stars. To get the space distribution of carbon stars we carried out near-infrared photometric observations and estimated total radiant energies (TRE) from individual carbon stars. By comparing the TRE with assumed intrinsic luminosity, distances of carbon stars are evaluated and then we obtained the space distribution of carbon stars. The space distribution of M-type stars is obtained by analyzing the photometric data of IRAS observations. Comparing the space distributions of carbon stars and M-type stars, we have found that two distributions are different from each other. This result shows that the evolutionary sequence of AGB stars is not the same in the whole galaxy.

Report

(3 results)
  • 1997 Annual Research Report   Final Research Report Summary
  • 1996 Annual Research Report

URL: 

Published: 1996-04-01   Modified: 2016-04-21  

Information User Guide FAQ News Terms of Use Attribution of KAKENHI

Powered by NII kakenhi