/ftp/cats/J_A+AS/140/309/.



==========================================================================
J/A+AS/140/309      Blue-Halpha objects in M33            (Fabrika+, 1999)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat
==========================================================================
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+AS/140/309
==========================================================================

drwxr-xr-x 14 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 2013 [TAR file] -rw-r--r-- 1 cats archive 463 Dec 17 2010 .message -r--r--r-- 1 cats archive 4181 Dec 16 2010 ReadMe -rw-r--r-- 1 cats archive 1007 Dec 17 2010 +footg5.gif -rw-r--r-- 1 cats archive 2501 Dec 17 2010 +footg8.gif -r--r--r-- 1 cats archive 16470 Oct 14 2010 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+AS/140/309 Blue-Halpha objects in M33 (Fabrika+, 1999) ================================================================================ A survey of blue - Halpha objects in the galaxy M33. Fabrika S., Sholukhova O. <Astron. Astrophys. Suppl. Ser. 140, 309 (1999)> =1999A&AS..140..309F ================================================================================ ADC_Keywords: Galaxies, nearby ; Stars, early-type ; Stars, blue Keywords: nearby galaxies: stellar content: individual (M33) - stars: early type - Halpha excess Abstract: For the purposes of a search for SS433 type objects, LBV stars and hypergiants in M33, we have carried out a photometry of blue stars in Halpha images of this galaxy. From 2332 listed OB stars, we have isolated 549 objects, which have Halpha excess over stars of the same V magnitude. Among them 81 emission stars (s) have been selected. About 60% of isolated objects found to be extended in Halpha, among them 154 diffuse (d) and 180 bubble-type (b) nebulae. 117 objects are compact (c) and faint Halpha sources. These groups are different in colour indices, Halpha fluxes, surface brightness and sizes. The most probable size of the Halpha nebulae is FWHM=10-14pc. There is evidence that their properties and location in the galaxy are defined by interstellar gas pressure and related to spiral arms. The d objects are HII regions with an embedded star. The b objects are probably envelopes around WR stars or SN remnants. Among s-type objects we isolated a group of 20 brightest stars, which in their average properties fit well to the parameters of blue hypergiants or LBV-type stars. The stars of intermediate brightness follow very well to blue Ia supergiants. The interstellar absorption derived from brightest Halpha stars is A_V_=0.93+/-0.05mag. We classify the faintest stars as blue Ib supergiants, their average absorption is A_V_ 0.6mag. They are restricted in number by the limiting stellar magnitude in the original sample. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 01 33 54.0 +30 40 07 M 33 = NGC 598 ------------------------------------------------

© UDS/CNRS

Contact