Steve Gottlieb
July 31st, 2013, 07:30 PM
7) LMC-N44 Complex
NGC 1929 (24"): this HII knot is the first in an impressive star cluster/emission complex (stellar association LH 47) that extends over 7' in size and includes NGC 1934, 1935, 1936, 1937, and IC 2126. At 260x it appeared as a bright, moderately large, round glow of ~50" diameter surrounding a 13th magnitude star.
On the DSS this object appears to be a symmetrical bubble. This HII complex and cluster includes the superbubble complex N44
NGC 1934 (24"): this is a locally brighter patch in the NGC 1929-34-35-36-37 complex (stellar association LH 47), situated very close northwest of NGC 1935. This patch is not as well defined as the other NGC objects in this bright HII complex but is noticeable as it involves a couple of brighter mag 12 stars and a number of fainter stars.
S-L 417 (24"): rich concentration of stars superimposed on the entire LMC-N44 complex, including the HII regions NGC 1929, 1934, 1935 and 1936 off the south side.
NGC 1935 (24"): this emission glow forms the NW pair with NGC 1936 in a very striking field of clusters and HII patches (part of stellar association LH 47). At 200x and UHC filter it appeared as a very bright, round glow of uniform high surface brightness. The size is slightly smaller than NGC 1936, perhaps 45"-50" in diameter. Good response to the UHC filter. Nebulosity also extends off to the NW of NGC 1935 and a locally brighter patch (NGC 1934) involves a couple of brighter stars. Superimposed on this entire complex of HII knots is a rich concentration of stars (S-L 417 = KMHK 822).
NGC 1936 (24"): NGC 1936 appeared as a very bright, round glow, ~1' diameter with a very high, uniform surface brightness at 200x using a UHC filter. Situated at the south end of a large cluster and HII complex. Additional fainter nebulosity sweeps to the south and is connected with a fainter (anonymous) patch to the west by 1'. This extension increases the total size to 2' to 2.5'. NGC 1935 lies 2' NW.
NGC 1937 (24"): this object is the furthest NE in a gorgeous field of stars and HII regions. NGC 1937 is a large nebulous patch, ~3.7'x2.7' in size, with ~20 stars resolved over the bright glow. Excellent contrast gain using a UHC filter at 200x. The cluster or star cloud (association LH 48) includes a string of stars oriented WSW-ENE that passes through the center including a mag 11 star. NGC 1936, a very bright nebulous glow, lies 5' S, and other sections of the N44 superbubble complex (see http://www.universetoday.com/am/publish/gemini_interstellar_cavern.html) lie to the SW including NGC 1929, 1935 and IC 2126. Superimposed on this complex of HII glows is a fairly rich concentration of stars.
IC 2128: Star cloud (Association LH 49) located at the SE end of the NGC 1929-1936 complex (LMC N44)
NGC 1929 (24"): this HII knot is the first in an impressive star cluster/emission complex (stellar association LH 47) that extends over 7' in size and includes NGC 1934, 1935, 1936, 1937, and IC 2126. At 260x it appeared as a bright, moderately large, round glow of ~50" diameter surrounding a 13th magnitude star.
On the DSS this object appears to be a symmetrical bubble. This HII complex and cluster includes the superbubble complex N44
NGC 1934 (24"): this is a locally brighter patch in the NGC 1929-34-35-36-37 complex (stellar association LH 47), situated very close northwest of NGC 1935. This patch is not as well defined as the other NGC objects in this bright HII complex but is noticeable as it involves a couple of brighter mag 12 stars and a number of fainter stars.
S-L 417 (24"): rich concentration of stars superimposed on the entire LMC-N44 complex, including the HII regions NGC 1929, 1934, 1935 and 1936 off the south side.
NGC 1935 (24"): this emission glow forms the NW pair with NGC 1936 in a very striking field of clusters and HII patches (part of stellar association LH 47). At 200x and UHC filter it appeared as a very bright, round glow of uniform high surface brightness. The size is slightly smaller than NGC 1936, perhaps 45"-50" in diameter. Good response to the UHC filter. Nebulosity also extends off to the NW of NGC 1935 and a locally brighter patch (NGC 1934) involves a couple of brighter stars. Superimposed on this entire complex of HII knots is a rich concentration of stars (S-L 417 = KMHK 822).
NGC 1936 (24"): NGC 1936 appeared as a very bright, round glow, ~1' diameter with a very high, uniform surface brightness at 200x using a UHC filter. Situated at the south end of a large cluster and HII complex. Additional fainter nebulosity sweeps to the south and is connected with a fainter (anonymous) patch to the west by 1'. This extension increases the total size to 2' to 2.5'. NGC 1935 lies 2' NW.
NGC 1937 (24"): this object is the furthest NE in a gorgeous field of stars and HII regions. NGC 1937 is a large nebulous patch, ~3.7'x2.7' in size, with ~20 stars resolved over the bright glow. Excellent contrast gain using a UHC filter at 200x. The cluster or star cloud (association LH 48) includes a string of stars oriented WSW-ENE that passes through the center including a mag 11 star. NGC 1936, a very bright nebulous glow, lies 5' S, and other sections of the N44 superbubble complex (see http://www.universetoday.com/am/publish/gemini_interstellar_cavern.html) lie to the SW including NGC 1929, 1935 and IC 2126. Superimposed on this complex of HII glows is a fairly rich concentration of stars.
IC 2128: Star cloud (Association LH 49) located at the SE end of the NGC 1929-1936 complex (LMC N44)