Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Yvette Andrillat"'
Autor:
Yvette Andrillat, Carlos Jaschek
Publikováno v:
International Astronomical Union Colloquium. 175:83-86
The star MWC 84 (CI Cam) was first discovered to be an emission line object classified Bep (Merrill & Burwell, 1933), then classified as a symbiotic star and finally identified as the possible optical counterpart of the X-ray transient XTE J0421+560
Autor:
C. Jaschek, Yvette Andrillat
Publikováno v:
Astronomy and Astrophysics Supplement Series. 136:53-58
On the basis of spectroscopic CCD material obtained at the Haute Provence Observatory, we provide line identifications and equivalent width measurements in the wavelength region 4086-8780 A of the spectrum of MWC 17. Four hundred emission features ar
Autor:
C. Jaschek, Yvette Andrillat
Publikováno v:
Astronomy and Astrophysics Supplement Series. 136:59-63
On the basis of spectroscopic CCD material obtained at the Haute Provence Observatory, we provide line identifications and equivalent width measurements in the wavelength region 4095-8935 A of the spectrum of MWC 342. Two hundred eighty emission feat
Autor:
E. L. Chentsov, Y. Frémat, Léo Houziaux, Anatoly S. Miroshnichenko, V. G. Klochkova, Yvette Andrillat
Publikováno v:
Astronomy and Astrophysics Supplement Series. 131:469-478
The results of high{resolution optical spec- troscopy obtained for a recently suggested LBV candidate, MWC 314, are presented. Photospheric lines mostly of N ii and S ii have been found for the rst time with a res- olution of 0:4 0:8 A. They imply a
Autor:
Yvette Andrillat, C. Jaschek
Publikováno v:
Astronomy and Astrophysics Supplement Series. 131:479-482
On the basis of spectroscopic CCD material obtained at the Haute Provence Observatory, we provide line identifications and equivalent width measurements in the wavelength region 4100 - 8900 A of the spectrum of MWC 297. About two hundred features are
Autor:
C. Jaschek, Yvette Andrillat
Publikováno v:
Astronomy and Astrophysics Supplement Series. 130:507-512
We present and discuss the observations of 14 Ae and A type shell stars in the visual, the Hα region and the near infrared. At least 57% of these stars are spectrum variables. The Paschen lines are formed in a region which has the characterics of gi
Autor:
C. Jaschek, Yvette Andrillat
Publikováno v:
Astronomy and Astrophysics Supplement Series. 128:475-483
On the basis of spectroscopic CCD material obtained at the Haute Provence Observatory, we provide line identifications and equivalent width measurements in the wavelength region 3738-10232 A of the spectrum of HD 50138 Over two hundred features are i
Publikováno v:
Astronomy and Astrophysics Supplement Series. 124:441-448
On the basis of spectroscopic CCD material obtained at the Haute Provence Observatory, we provide line identifications and equivalent width measurements in the wavelength regions 3750-5112 and of the spectrum of HD 45677. Over 235 features are identi
Publikováno v:
Astronomy and Astrophysics Supplement Series. 120:99-105
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide identifications and equivalent width measurements in the wavelength region 3740-8790. About 350 emissions lines were measured and about 88 of them were ident
Publikováno v:
Astronomy and Astrophysics Supplement Series. 118:495-502
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide line identications and equivalent width measurements in the wavelength region 3700 8790 A. Over 300 emission features are identied and a comparison of our re