Open AccessLuminous variables in the Quintuplet cluster
Author(s) -
Glass I. S.,
Matsumoto S.,
Carter B. S.,
Sekiguchi K.
Publication year - 1999
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1999.02454.x
Subject(s) - physics , astrophysics , luminous blue variable , variable star , astronomy , stars , globular cluster , star cluster , line of sight , open cluster
We report observations of variability amongst the stars of the `Quintuplet' cluster located about 30 pc in projection from the centre of the Galaxy. Two of the five cocoon star members, which may be protostars or peculiar Wolf‐‐Rayet stars, are seen to vary slowly with moderate amplitude (0.4‐‐0.5 mag). The bright star within the `Pistol' H ii region, suspected of being a luminous blue variable (LBV), has in fact been found to show variability, confirming its tentative classification. A second nearby presumed LBV also varies. One of the apparent Quintuplet members is likely to be a Mira variable along the same line of sight.