Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range
Publikation: Bidrag til bog/antologi/rapport › Bidrag til rapport › Formidling
Standard
Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range. / Loidl, R.; Hron, J.; Jørgensen, U.G.; Höfner, S.
Conf. proceedings: ISO beyond the Peaks: The 2nd ISO workshop on analytical spectroscopy, ESA SP-456. 2001. s. 315-318.Publikation: Bidrag til bog/antologi/rapport › Bidrag til rapport › Formidling
Harvard
Loidl, R, Hron, J, Jørgensen, UG & Höfner, S 2001, Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range. i Conf. proceedings: ISO beyond the Peaks: The 2nd ISO workshop on analytical spectroscopy, ESA SP-456. s. 315-318.
APA
Loidl, R., Hron, J., Jørgensen, U. G., & Höfner, S. (2001). Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range. I Conf. proceedings: ISO beyond the Peaks: The 2nd ISO workshop on analytical spectroscopy, ESA SP-456 (s. 315-318)
Vancouver
Loidl R, Hron J, Jørgensen UG, Höfner S. Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range. I Conf. proceedings: ISO beyond the Peaks: The 2nd ISO workshop on analytical spectroscopy, ESA SP-456. 2001. s. 315-318
Author
Bibtex
@inbook{5bb15c4074be11dbbee902004c4f4f50,
title = "Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range",
author = "R. Loidl and J. Hron and U.G. J{\o}rgensen and S. H{\"o}fner",
year = "2001",
language = "English",
pages = "315--318",
booktitle = "Conf. proceedings: ISO beyond the Peaks: The 2nd ISO workshop on analytical spectroscopy, ESA SP-456",
}
RIS
TY - GEN
T1 - Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range
AU - Loidl, R.
AU - Hron, J.
AU - Jørgensen, U.G.
AU - Höfner, S.
PY - 2001
Y1 - 2001
M3 - Report chapter
SP - 315
EP - 318
BT - Conf. proceedings: ISO beyond the Peaks: The 2nd ISO workshop on analytical spectroscopy, ESA SP-456
ER -
ID: 16666