UBV photometry of OB associations within superbubbles of the
Large Magellanic CloudJ/ApJS/104/71J/ApJS/104/71UBV photometry of OB associations in LMC superbubblesUBV photometry of OB associations within superbubbles of the
Large Magellanic CloudMSOeyAstrophys. J. Suppl. Ser.1047119961996ApJS..104...71OH II regionsMagellanic CloudsNebulaePhotometry, UBVHII regionsISM: bubblesMagellanic Cloudsopen clusters and associations: general
Tables 4a-m provide the photometry for the OB associations of the
sample, including both superbubbles and diffuse H II regions. Notes
for individual objects are:
DEM 31: Photometry for D31-2001 (Sk -67 17) listed from
Ardeberg et al. (1972A&AS....6..249A)
DEM 106: Stars with prefix D106A- have V photometry from a separate,
short exposure.
DEM 192: Stars with prefix D192A- have V photometry from a separate,
short exposure.
DEM 301: Photometry for D301-1005 listed from Massey et al.
(1995ApJ...438..188M) Postscript versions of the plates in Figure 1 of the printed paper
are included. Each is a V image of the OB association field,
with bright stars identified. The remaining stars can be identified
with the aid of coordinates given in Table 4a-m. Each individual
frame is 3.8' x 3.8' square, with north up and east to the left.
This work presents UBV photometry of the stellar populations
associated with seven superbubble nebulae and five classical H II
regions in the Large Magellanic Cloud. Although the nebular morphology
of the superbubbles appears to be substantially evolved compared to
the classical nebulae, the color-magnitude diagrams do not reveal any
noticeable correlation between the resident stellar population and
nebular morphology. The photometry presented here will be used in a
forthcoming paper to examine further the stellar content and dynamics
of these superbubbles.Photometry for DEM 25Photometry for DEM 31Photometry for DEM 50Photometry for DEM 106Photometry for DEM 192Photometry for DEM 226Photometry for DEM 231Photometry for DEM 301Photometry for DEM 10bPhotometry for DEM 66Photometry for DEM 197Photometry for DEM 243Photometry for DEM 293IDStar identification
Star identification. Stars with a and b components are
spectroscopic binaries, whose V magnitude has been estimated as
described in the printed paper. However, the colors listed for both
components are the original, combined colors determined for the
composite object. The DAOPHOT errors for these objects are
misleading, and have been deleted.---RAhRight ascension (2000.0)hRAmRight ascension (2000.0)minRAsRight ascension (2000.0)sDE-Declination sign---DEdDeclination (2000.0)degDEmDeclination (2000.0)arcminDEsDeclination (2000.0)arcsecVmagV magnitudemage_VmagError in Vmag
These are the photometric errors computed by DAOPHOT and do not
include systematic effects such as those introduced by aperture
corrections and transformation errors.
magB-VB-V colormage_B-VError in B-VmagU-BU-B colormage_U-BError in U-Bmagfigure1a.psV image for DEM 25figure1b.psV image for DEM 31figure1c.psV image for DEM 50figure1d.psV image for DEM 106figure1e.psV image for DEM 192figure1f.psV image for DEM 226figure1g.psV image for DEM 231figure1h.psV image for DEM 301figure1i.psV image for DEM 10bfigure1j.psV image for DEM 66figure1k.psV image for DEM 197figure1l.psV image for DEM 243figure1m.psV image for DEM 293CDS1996Sep06AAS CD-ROM series, Volume 6, 1996 Lee Brotzman [ADS] 03-May-96J_ApJS_104_71.xml