196 



OBSERVATIONS ON NEBULiE 



No. 



Mag. 



R. A. 1830.0 



Decl. 1830.0 



121 



10.11 



20'' 49'" 54^41 



+ 30= 



45' r2".8 



122 



12.13 



" 54 .9 



it 



49 24 



123 



15 



" 55 .5 



(( 



25 6 



124 



12.13 



" 57 .7 



6( 



52 8 



125 



15 



" 58.1 



ii 



23 52 



126 



14.15 



" 58 .4 



(( 



23 7 



127 



14.15 



" 58.9 



(( 



80 33 



128 



14 



" 59.2 



(( 



42 53 



129 



10.11 



" 59.46 



<( 



47 13 



130 



10.11 



" 59 .48 



31 



10 3 .6 



131 



14.15 



" 50 1 .6 



30 



27 26 



132 



14.15 



" 1.7 



It 



31 26 



133 



10.11 



1 .89 



(1 



28 44 .0 



134 



12.13 



" 2.5 



n 



53 40 



135 



14 



" 2.5 



ti 



31 45 



136 



12.13 



" 2.6 



31 



4 19 



137 



14.15 



" 2.6 



30 



23 10 



138 



13 



" 2.7 



31 



59 



139 



12.13 



" 5.9 



ti 



1 6 



140 



14.15 



" 6.1 



30 



42 52 



141 



10.11 



" 6.1 





11 46 



142 



14 



" 6.6 





18 11 



143 



14 



0.9 





40 36 



144 



11 



" 7 .2 





52 39 



145 



15 



" 7.8 





32 30 



146 



12 



" 8.2 





49 26 



147 



12.13 



" 8.3 





23 3 



148 



14.15 



" 8.4 





42 52 



149 



16 



" 9.0 





22 40 



150 



15 



" 9.4 





29 49 



151 



14.15 



» 9.4 





29 8 



152 



13 



" 10.3 





22 52 



153 



13 



" 11.3 





23 5 



154 



14.15 



" 11.7 





29 23 



155 



12 



" 11.9 





54 12 



156 



10 



" 12.2 





23 8 



157 



14 



" 13.6 





18 13 



158 



14 



" 14.0 





25 50 



No. 



Mag. 



K. A. 1830.0 



Decl. 1830.0 



159 



14 



20>' 50'" 15^3 



+ 30" 



40' 23". 



160 



12.13 



" 16.1 





51 35 



161 



13 



" 16.6 





40 41 



162 



10.11 



•' 16 .77 





28 56 



163 



12 



" 18.1 





43 13 



164 



14 



" 18.5 





26 50 



165 



14 



" 18.5 





41 56 



166 



12.13 



" 19.4 





34 14 



167 



13 



" 20 .2 





26 6 



168 



14 



" 21 .4 





33 13 



169 



13 



" 24 .0 





29 38 



170 



13 



" 26.6 





33 12 



171 



14.15 



" 29 .2 





17 26 



172 



14 



" 32.1 





28 18 



173 



12.13 



" 32 .2 





16 24 



174 



12.13 



" 33 .3 





18 3 



175 



14 



" 34.6 





34 24 



176 



10 



" 34 .58 





38 20 .3 



177 



13 



" 35 .0 





33 51 



178 



14 



" 35 .7 





27 17 



179 



12 



" 38 .7 





13 34 



180 



12.13 



" 42 .7 





33 4 



181 



14 



" 44 .8 





39 53 



182 



12.13 



" 49 .4 





35 



183 



10.11 



" 52 .49 





19 13 



184 



12 



" 53 .6 





20 1 



185 



12.13 



«« 56 .9 





32 36 



186 



13 



" 57 .0 





28 11 



187 



8.9 



" 59 .66 





38 54 .6 



188 



12.13 



" 59 .8 





20 54 



189 



14 



51 0.1 





21 30 



190 



9.10 



" .30 





42 8 .0 



191 



11 



" 2 .7 





28 19 



192 



11 



" 3.2 





29 30 



193 



10.11 



" 4 .62 





15 12 .5 



194 



11 



" 10.8 





26 41 



195 



12 



" 21 .3 





18 46 



196 



11 



" 22 .7 





18 22 



40. Of these three catalogues the first is probably the most correct. The 

 stars in nebula h. 2008 are less determinate. This is chiefly due to the some- 

 what hurried completion of the map of that nebula in the month of August, 

 the moon becoming troublesome sooner than was altogether convenient. And 

 for the purposes of correction, only two or three stars exist in, or very near this 

 nebula, of a magnitude as great as the eleventh; so that it was necessary to 

 place reliance on the extremely difficult measures of the twelfth and thirteenth 

 magnitudes. 



But one set of measures in Decl. were taken of star (193) in the large nebula, 



