VizieR

Distance ρ
Position angle θ
Distance (x,y)
Galactic
J2000
B1950
Ecl. J2000

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If the access to catalogues with VizieR was helpful for your research work,the following acknowledgment would be appreciated: This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in A&AS 143, 23

	J/A+A/585/A141	4062		Galactic center early-type stars catalog (Grosboel, 2016) ReadMe+ftp 2016A&A...585A.141G Similar Catalogs spectrum/fits [ets_tgc.fit] spectrum/fits
	J/A+A/585/A141/ets_tgc		^(c)Catalog of early-type stars toward the Galactic center (12675 rows)
	J/MNRAS/488/1090	-1		Unclassified B[e] stars in the MW, SMC and LMC (Condori+, 2019) ReadMe+ftp 2019MNRAS.488.1090C Similar Catalogs
	J/MNRAS/488/1090/table1		^(c)Our sample of unclassified B[e] stars and candidates observed with FEROS (30 rows)
	J/MNRAS/488/1090/table2		^(c)Photometric data of our sample collected from the literature (27 rows)
	J/MNRAS/488/1090/table3		^(c)The radial velocity of stars from our sample that do not present sensible spectral variability or for which we have just one spectrum (14 rows)
	J/MNRAS/488/1090/table4		^(c)Radial velocities, derived from permitted absorption and forbidden emission lines, for the objects with strong variability (13 rows)
	J/MNRAS/488/1090/table5a		^(c)Spectral type, luminosity class, intrinsic color index, and effective temperature for some stars of our sample, obtained using method 1 (9 rows)
	J/MNRAS/488/1090/table5b		^(c)Spectral type, intrinsic color index, and effective temperature for some stars of our sample, obtained using method 2 (7 rows)
	J/MNRAS/488/1090/table5c		^(c)Effective temperature for some stars of our sample, obtained using method 3 (3 rows)
	J/MNRAS/488/1090/table6		^(c)Interstellar, circumstellar, and total color excess, E(B-V), and visual interstellar extinction, A_V, for the objects of our sample (12 rows)
	J/MNRAS/488/1090/table7		^(c)Velocities needed for fitting the line profiles for the stars with both [OI] and [CaII] forbidden lines (5 rows)
	J/MNRAS/488/1090/table8		^(c)Velocities needed for fitting the line profiles for the stars with only the [OI] forbidden lines (16 rows)
	J/MNRAS/488/1090/table9		^(c)Physical parameters of the stars of our sample (11 rows)
	J/MNRAS/500/3926	-1		Optical spectroscopy of classical Be stars (Banerjee+, 2021) ReadMe+ftp 2021MNRAS.500.3926B Similar Catalogs
	J/MNRAS/500/3926/table1		^(c)List of our program CBe stars and the log of observations (138 rows)
	J/MNRAS/500/3926/table2		^(c)Our adopted distance for 83 of our sample stars whose parallax values are available in Gaia DR2 and their re-estimated A_V values (83 rows)
	J/MNRAS/500/3926/table3		^(c)List of 35 of our program stars for which A_V values are adopted from the literature (35 rows)
	J/MNRAS/500/3926/table4		^(c)Estimated Balmer decrements, D₃₄ and D₅₄ for our program stars (115 rows)
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			^(c) indicates tables which contain celestial coordinates

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