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DOCdb - NGC 1513

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NGC 1513

NGC 1513, Cl Collinder 46, C 0406+493, VII 60, GC 809

RA: 04h 09m 55s
Dec: +49° 31′ 0″

Con: Perseus
Ch: MSA:76, U2:64, SA:5

Ref: SIMBAD, Collinder (1931), DAML02, Archinal&Hynes (2003), Skiff20080430-s

(reference key)

Type: open cluster, 21m

Mag: B=8.71, V=8.4

Size: 10′
PA: ?

Historical observations

William Herschel (c.1784)

Synonyms:H VII-060

Discovered in 1790 by William Herschel with an 18.7-inch f/13 speculum telescope. He called it "a large cluster of cL stars, pretty compressed and very rich, iR, 7' diameter."

Published comments

Trumpler, R.J. (1928)

Trumpler (Lick Obs. Bulletin, Vol 14, No 420) gives the diameter as 9' and the class as 2 2 m. He notes that it is markedly unsymmetrical.

Sulentic & Tifft (1973)

The RNGC (Sulentic and Tifft 1973) notes that this is a 9.0 mag open cluster.

Modern observations

Ancient City Astron.Club (1980)

Listed by the Herschel Club, described as "counted 40 stars, slightly loose grouping outwards from a compact nucleus, well defined. 8-inch, 48x."

Gross, Todd (IAAC)

Observer: Todd Gross Your skill: Intermediate Date and UT of observation: 11/5/97 0800 GMT Location & latitude: 22 miles west of Boston, Ma. 42.3N Site classification: Suburban Limiting magnitude (visual): 5.2 (estimated) 5.2 (est) in vicinity of object Seeing (1 to 10 - worst-best): 8 Moon up (phase?): No Weather: Clear Instrument: 16" Newtonian-dob w. 96/99% coatings f/4.59 Magnifications: 124x Filters used: none Object: NGC 1513 Constellation: Object data: Open Cluster Personal rating (at this aperture): B

"NGC 1513 is a most interesting mid-sized open cluster with a myriad of dim stars. For the lack of being able to describe it better, the cluster looks like two breasts. That is, two bags of stars (I believe pointing SOUTH) the easternmost bag is simply a circle of dim stars with a dim star inside as well. The westernmost bag is more irregular shaped. Both are connected on the North side. While I did not confirm this, I think it probably is best in larger aperture because of the lack of bright members."

Tom Lorenzin

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: "9M; 12' diameter; large, very rich, and much compressed; 40-plus 11M and dimmer members."

Steve Gottlieb

& Cr 46 & OCL-398 & Lund 125

04 09.9 +49 31

13: about 60 stars mag 11 and fainter over unresolved background glow.

Located 50' SE of Lambda Persei (V = 4.3).

Contemporary observations

Tom Bryant

2011 2 10 20:7:16

Observing site: Little Tycho Observatory

Telescope: C-8

[4h 10m 0s, 49° 31m 0s] 6 9-10 mv stars surround by a nebulous glow, which might just be the milky way. Not a great sight, on this moonlit night.


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