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Astronomy & Astrophysics, 1999
ORFEUS far UV echelle spectra have been used to investigate HI, Hz and CO absorption lines along the line of sight towards LH 10:3120 in the LMC, extending the study presented by de Beer et al. (1998). While Hz absorption is clearly visible, no CO absorption at LMC velocities is detected, but an upper limit of N(CO) less than or equal to 3.3 x 10(13 ...
Richter, P +5 more
openaire +1 more source
ORFEUS far UV echelle spectra have been used to investigate HI, Hz and CO absorption lines along the line of sight towards LH 10:3120 in the LMC, extending the study presented by de Beer et al. (1998). While Hz absorption is clearly visible, no CO absorption at LMC velocities is detected, but an upper limit of N(CO) less than or equal to 3.3 x 10(13 ...
Richter, P +5 more
openaire +1 more source

