1833.] visible in the Horizon of Calcutta. 255 
cS TS ES LE 
1 r= U U 1! s 
“Oo 3 Oy = 
< me = 3 w| 2s Description of Object. a S r) 
9 | 33 = ish og ° 
fe A IA| <a © Ne al 
h.m. 8. 
51}11 11 30)13 56/N.|M. 66] N.j|A very bright lengthened ne-|Leo. 13 
bula. 
*52112 1650/62 7:S.|a’ 123! D. Ja Crucis,2nd class. Thebrightest! Crux. 20 
and most remarkable double 
very large and splendid globu-| rus. 
lar cluster—the finest in the 
southern hemisphere. 
star in the southern hemis- 
pheret. Barely rises above the 
Calcutta horizon, high enough 
to be tolerably well seen. 
+ a Centauri excepted. 
53|12 27 52|2655|N.|v. 24| N. 1A long sword-shaped nebula. Coma 7 
Beren. 
*54)12 33 3) 031)S. D. |v Virginis. One of the most re-|Virgo. [14 
markable of the Binary stars. 
Period of revolution 513 years. 
Close and difficult, and becom- 
ing more so. 
*55/12 33 56/33 29|N.|/V. 42] N. |A very long narrow nebulous|Canes 7 
ray. Venatici. 
56|1247 9/39 16|N. D. ja Canum. Cor. Caroli, 4th class.|Canes 7 
Contrasted colours. Ven. 
57|12 48 32|22 361N.|M. 64| N. |A nebula with a nucleus and a|Coma 7 
| black recess. Ber. 
58)13 447|19°7|N.IM. 53) @® B condensed globe of stars. out { 7 
. er 14 
59|13 7 4/4258'N.i1M. 63] @ 1A very bright extended mass of|Canes 7s 
stars like the finest dust. Ven. 
60/1315 3)2858|S.|a 628] @ |A globular cluster suddenly con-|Centau- {19 
, densed toward the centre to an} rus. 
extraordinary degree. 
**61,1316 0/46 34/S.;Aa - @® |w Centauri—not a star, but a]Centau- {19 
**62113 22 i, 3|N.|M. 51] © JA most wonderful object. A/Canes 7 
globe surrounded by a dou-| Ven. 
ble ring of nebulax—It has a 
| neb. near it, as a compani- 
on. It is unique in the hea- 
| | vens. 
6313 34 49129 13)N.|M. 3] @ \* much compressed cluster. Canes 7 
Ven. 
64/13 58 11/55 13)N.|M.101, N. JA very bright nebula. Ursa 6 
Maj. 
65|14 10 27157 40|S.|A’ 159| D. !y Centauri, 3rd class, 5 and 8 m.|Centau- |20 
rus. 
*66|14 28 0|60 6|S.|A’ 165] D. |a Centauri, 4th class,1st and 4th|Centau- |20 
magnitudes. Distance 19.” The! rus. 
| brightest double star in the S. 
hemisphere. Very low in the 
| S. horizon, but may be occasi- 
onally pretty well seen. 
