Infrared spectra of ZrC presolar grain analogues

Y. Kimura, C. Kaito

Research output: Contribution to journalArticlepeer-review

1 Citation (Scopus)

Abstract

The origins of spectral feature of stellar source are identified on the basis of laboratory studies. Although ZrC grains were identified as the crystalline presolar grains in meteorites, the spectral data of ZrC grains have not been measured in the laboratory. Therefore, ZrC grains with the same size as the presolar grains were produced in the laboratory. It has been found that the infrared spectrum of ZrC grains shows broad absorption features at 9.4 and 12.4 μm.

Original languageEnglish
Pages (from-to)159-161
Number of pages3
JournalAstronomy and Astrophysics
Volume409
Issue number1
DOIs
Publication statusPublished - 2003 Oct

Keywords

  • ISM: general
  • Infrared: ISM
  • Infrared: stars
  • Stars: AGB and post-AGB
  • Stars: carbon
  • Stars: circumstellar matter

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Infrared spectra of ZrC presolar grain analogues'. Together they form a unique fingerprint.

Cite this