NGC 7479 - Barred Spiral Galaxy


Designations:
NGC 7974, Caldwell C44, H I 55, UGC 12343, IRAS23024+1203, PGC 70419
Object Type:
Barred Spiral Galaxy
Constellation:
Pegasus
23 hr 4 min 47.1 sec
+12° 19 min 18 sec
10.9
Size:
4.4 X 3.4 arcminutes
Distance:
100 million light years

Visual Description:

NGC 7974 is probably the best barred spiral galaxy in the northern hemisphere and, at a visual magnitude of 10.8, is bright enough to be visible in modest telescopes. Orientated almost face-on, an 8 inch (20cm) telescope shows a cigar shaped object about 4 arc-minutes long by 1 wide, running almost due north-south. This is NGC 7974's prominent bar and averted vision shows some mottling in it, possibly due to the dust lanes in the bar. However the two spiral arms, which emanate from each end of the bar, requires more aperture. A 16 inch reveals the western arm but even in this telescope the eastern one is still invisible. The nucleus is however obvious and looks like a 12th magnitude star. NGC 7974 is very easy to find, being 3° due south of Alpha Pegasi (Markab).

NGC 7974 is a classical barred galaxy, almost face-on with the spiral arms winding out from a very prominent bar. As a result NGC 7974 has been extensively studied in order to understand bar formation. Also in its favor is its isolation from other galaxies and its morphology is therefore due solely to itself rather than any galactic interactions. So understand NGC 7974 and take a large step to understanding barred spirals. To do this it is necessary to study its interstellar material ( and NCG 7974 has plenty ) as well as just its stars. Laine et al. (1988 & 1999) used radio telescopes primarily to detect emissions from CO (carbon monoxide molecules), which are easier to observe than H-alpha but are believed to be accurate tracers of it. CO emissions were detected only in the dust lane that runs the length of the bar. Results indicate that the motion of the molecular gas is circular in the circum-nuclear region but outside this there is a strong radial velocity, inward towards the nucleus. Laine and Gottesman (1997) proposed that the more prominent western arm was the result of a minor merger. Rozas et al. (1999) on the other hand examined NGC 7974 in H-alpha light detecting over 1,000 H-II regions with only a small number in the bar.




Telescope:
Meade 10" LX200 Optical Tube Assembly
Focal Length:
2500 mm
Mount:
Camera
Starlight XPress MX916
Guider:
Starlight XPress S.T.A.R 2000 Autoguider
Exposures:
8 15-minute exposures
Location:
Software:



The visual descriptions of NGC 7479 was written by David Ratledge in the book "Observing the Caldwell Objects" by David Ratledge. Page 102.
ISBN number 0-85233-628-5.






Copyright(c) 2009 Doug Sanqunetti All rights reserved.

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