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19942003
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astro-ph2003

The far infrared CO line emission of Orion BN/KL

S. Maret, E. Caux, J. P. Baluteau +3

We present observations towards one of the closest regions of high mass star formation, Orion BN/KL, performed at both low resolution mode (grating mode) and high resolution mode (…

astro-ph2001

FUSE Observations towards HD 34078 Detection of highly excited H2 and HD

Franck Le Petit, Patrick Boisse, Guillaume Pineau des Forets +4

We present FUSE observations of the extincted O9.5 star, HD 34078. The 19 first levels of H2 are detected (i.e. from J=0 to v=1, J=5) as well as HD in its two first levels. The exc…

astro-ph2000

Electron densities, temperatures and ionization rates in two interstellar clouds in front of beta Canis Majoris, as revealed by UV absorption lines observed with IMAPS

Edward B. Jenkins, Cecile Gry, Olivier Dupin

The spectrum of beta CMa (Mirzam) between 1000 and 1200 A was recorded at a wavelength resolving power ~ 60 000 by the Interstellar Medium Absorption Profile Spectrograph (IMAPS) d…

astro-ph1997

EROS Variable Stars : Discovery of Beat Cepheids in the Small Magellanic Cloud and the effect of metallicity on pulsation

J. P. Beaulieu, M. Krockenberger, D. D. Sasselov +27

We report the discovery of eleven beat Cepheids in the Small Magellanic Cloud, using data obtained by the EROS microlensing survey. Four stars are beating in the fundamental and fi…

astro-ph1996

Metallicity Effects on the Cepheid Extragalactic Distance Scale from EROS photometry in LMC and SMC

D. D. Sasselov, J. P. Beaulieu, C. Renault +30

This is an investigation of the period-luminosity relation of classical Cepheids in samples of different metallicity. It is based on 481 Cepheids in the Large and Small Magellanic…

astro-ph1996

The effect of metallicity on the Cepheid distance scale and its implications for the Hubble constant () determination

J. P. Beaulieu, D. D. Sasselov, C. Renault +30

Recent HST determinations of the expansion's rate of the Universe (the Hubble constant, H_0) assumed that the Cepheid Period-Luminosity relation at V and I are independent of metal…