Spectroscopic Identification of White Dwarfs in Galactic Clusters - Part Six - Three New White Dwarfs in NGC3532

Details Spectroscopic Identification of White Dwarfs in Galactic Clusters - Part Six - Three New White Dwarfs in NGC3532 Spectroscopic Identification of White Dwarfs in Galactic Clusters - Part Six - Three New White Dwarfs in NGC3532

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...275..479k&link_type=abstract

Astronomy and Astrophysics, Vol.275, NO.2/AUG(II), P. 479, 1993

Astronomy and Astrophysics

Astrophysics

26

Open Clusters And Associations: Ngc 3532, Stars: White Dwarfs

Scientific paper

We present new observations of seven white dwarf candidates in the galactic cluster NGC 3532. Three are spectroscopically confirmed to be hot white dwarfs and cluster members. Two of them have masses close to 0.6 Msun, close to the average mass of field white dwarfs, whereas the mass of the third is about 0.9 Msun. Progenitor masses in the range from 3.6 to 5.7 Msun are derived from the cooling ages and the age of the cluster.

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