Oxygen abundance in the old clusters of the Large Magellanic Cloud: ESO 121-SC03 and NGC 2210

Details Oxygen abundance in the old clusters of the Large Magellanic Cloud: ESO 121-SC03 and NGC 2210 Oxygen abundance in the old clusters of the Large Magellanic Cloud: ESO 121-SC03 and NGC 2210

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001newar..45..557s&link_type=abstract

New Astronomy Reviews, Volume 45, Issue 8, p. 557-558.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

As a part of the Science Verification of UVES, five giant stars in the two old clusters of the LMC ESO 121-SC03 and NGC 2210 were observed with UVES, the high resolution échelle spectrograph recently commissioned on the VLT of ESO. The oxygen abundance has been measured in these two old clusters and compared to the oxygen abundance measured in our Galaxy and in the young matter of the LMC.

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