The Leo Three

The Leo Three

The Leo Three
Sketch by Janis Romer, Details by Frank McCabe

Janis has rendered here an impressive sketch of the “Leo triplet” of galaxies in the constellation of the same name. The northern most member closest to the bottom of the drawing is NGC 3628. At approximately magnitude 9.9 visually, it was missed by Charles Messier but recorded by William Herschel in the spring of 1784. At 35 million light years distant it has an apparent diameter of 15 arc minutes. In an 18 inch telescope from good skies the dust lane bisecting this galaxy is clearly visible. The outer visible parts of this galaxy are distorted by gravitational interactions with the other two members of this group, namely M-65 and M-66. These two galaxies were discovered and recorded by Charles Messier in March of 1780 (incorrectly attributed to Pierre Mechain until recently corrected). M-65 the fainter of these two at magnitude 9.3 and western most (top left) in this sketch, is a tightly wound spiral with an apparent size of 8’ by 2’. M-66 the eastern most (top right) galaxy in the sketch is dusty looking and brighter at magnitude 8.9. This less symmetrical spiral measures 8’ by 3’ in apparent dimensions. Values for the distances of these last two galaxies vary from 22 million light years to 35 million. Measurements taken using Cepheid variables as standard measuring candles find the distance to these galaxies at about 35 million light years (11 mega parsec).

This sketch was made using a Criterion 8” f / 8 Newtonian reflector telescope

Galaxy Cluster Choreography

Stephan’s Quintet

Stephan’s Quintet
Sketch and Details by Dale Holt

Stephan’s Quintet

Perhaps as a follow on to Jeff Young’s superb NGC 7331 “Deer Lick with fleas” My own rendition of Stephan’s Quintet might fit well?

On the 2nd of October this year I used my observatory 14″ F5 Newt with Watec 120n video camera sketching from a 9″ B&W monitor, using a graphite pencil plus blending stump on standard cartridge paper to capture the enigmatic Stephan’s Quintet.
The image was scanned and turned to a negative to give a more realistic and pleasing view. I caught up with this exquisite galaxy cluster following some wonderful shared visual studies with my 20″ at the Kelling Heath Autumn Equinox star party in Norfolk, England the previous week.

Deer Lick with Fleas

Deer Lick Group

NGC7331 and 3 Fleas (7335, 7337, 7340)
Sketch and Details by Jeff Young

NGC7331 and 3 Fleas (7335, 7337, 7340)

galaxy group in Pegasus

sketched from County Louth, Ireland

as viewed through 16” Mak-Cass @ 150X

These guys are a particular favourite of mine — even when transparency isn’t great there’s NGC7331 to look at, and when the skies are better one can hunt for the Fleas. They’re also a good measure of nearby Stephan’s Quintet — if you can’t see any of the fleas you’re unlikely to be able to pull in the Quintet.

This sketch captures 3 of the 4 fleas; the one I missed (NGC7336) is between the upper flea and the row of 3 stars above it. The largest Flea near the centre was the easiest of the three — the other two required a look at 335X to distinguish from very dim stars.

Derwent HB Sketching pencil on 150gsm cartridge paper. (I’ve since moved to a slightly softer pencil as I found Derwent’s HB too hard.)

Hickson 68: Galaxy Cluster in Canes Venatici

Hickson 68

Hickson 68

Sketch and Details by Bill Ferris

Move mouse over sketch to see labels.

Hickson 68: Galaxy Cluster (Canes Venatici)

RA: 13h 53.5m / DEC: +40º 17′.0

Instrument: 18-inch Obsession

Here’s a fine galaxy cluster that adorns the spring sky. Hickson 68 resides in eastern Canes Venatici and is closer to the bright stars of Boötes than to Cor Caroli. My sketch presents a 199X view in the big Obsession and is dominated by NGC 5350. This 11.3 magnitude barred spiral is northernmost in the group and has the designation, Hickson 68C. Its stellar core is embedded within a 3′.3 by 2′.4 oval nebulosity that becomes gradually brighter toward the middle. The bright stellar pair immediately west of NGC 5350 are 6.5 magnitude HD 121197 and 10.5 magnitude PPM 53793. A skosh more than 4′ south of Hickson 68C, resides a pair of galaxies sharing the same patch of sky. NGC 5353 is Hickson 68A. It is the larger and, at 10.9 magnitude, brighter of the pair. Its 2′.7 by 1′.5 oval form is aligned northwest to southeast and features a stellar core. Hickson 68B (NGC 5354) lies an arcminute to the north. Just the bright inner core of this 11.3 magnitude gotham is seen. The 1′ circular patch of haze is anchored to the sky by a faintly stellar core. Two galaxies are stationed to the east of center in my drawing. NGC 5355 (Hickson 68D) stands about 5′ west of NGC 5350. This 1′.2 by 0′.7 galaxy shines at 13.1 magnitude and is aligned north-northeast to south-southwest. NGC 5358 is the most challenging member of Hickson 68. Hickson 68E is a 14.6 (B) magnitude galaxy. It appears 1′.5 by 0.5 in size and is arranged northwest to southeast. A close pair of 13th magnitude GSC stars simmer an arcminute to the southwest.

Draco’s Four Pack

Hickson 80

Hickson 80
Sketch and Details by Bill Ferris

Hickson 80: Galaxy Cluster (Draco) RA: 15h 59.3m / DEC: +65º 14′.0
Instrument: 18-inch Obsession

The four-pack of faint galaxies in my sketch comprise the compact galaxy cluster, Hickson 80. A pair of 14th magnitude stars stand separated by just 30″ near the center of the field. Hickson 80A and 80B, paired to the north, appear to mirror that stellar duo. Hickson 80A is the 15.7(B) magnitude sliver covering a 0′.8 by 0′.2 area and aligned roughly north-south. It is cataloged as 2MASX J15591912+6513579, according to the NASA/IPAC Extragalactic Database (NED). Hickson 80B (=PGC 56590) is the tiny, 16.4(B) magnitude smudge just 30″ to the south. Hickson 80C lies an arcminute due west of 80A. It is a 16.1(B) magnitude galaxy cataloged as PGC 56572. The most challenging member of the quartet is 16.8(B) magnitude Hickson 80D. This faint little stinker resides 50″ southeast of Hickson 80C and is only visible with averted vision. You’ll find this collection banished to the far northern reaches of the heavens, in Draco.

Galactic Queue

Markarian’s Chain

Markarian’s Chain
Sketch and Details by Ernest Shekolyan

Hi!

Let me contribute to ASOD one of my pictures

That is Markarian`s chain as it was seen 9/10 apr. 2007 in eyepiece of my scope at village Shumba, 50 km from St.Petersburg, Russia. That was visual limit 6.2m.

10″ Starfinder, 24 mm UWA, 46x, FOV: 105 ang. minutes, graphite pencil, white paper, then photocopy + level correction, crop and inverting in ACDSee

Sincerely yours, Ernest Shekolyan

Bright Gem in Virgo’s Collection

M58

M58, Virgo Cluster Galaxy
Sketch and Details by Jeremy Perez

M58 was my final Virgo Cluster galaxy observation on the evening of July 25. The core was faintly stellar and had a soft plateau of brightness that then dropped off gradually at the edges. It was mildly elliptical at a PA of about 70 degrees. The NGCIC project database notes a PA of 95 degrees. Checking the DSS Image shows the extended outer halo aligning reasonably well to 95 degrees. The inner core region however does line up closely to 70 degrees and is certainly the only portion I actually saw that night.

Object Information:

As with its neighbors, M58 lies about 60 million light years away. It is one of the brightest members of the Virgo Cluster of Galaxies. Charles Messier discovered M58 on April 15, 1779 along with M59 and M60 while observing the comet of 1779.

M58 is also cataloged as: NGC 4579, UGC 7796, MCG+02-32-160, CGCG 070.197, h 1368, GC 3121, VCC 1727, IRAS 12351+1205, PGC 42168

Subject M58 (NGC 4579)
Classification* Spiral Galaxy (Sb)
Position* Virgo [RA: 12:37:43.5 / Dec: 11:49:05]
Size* 5.9′ x 4.7′
Brightness* 10.1 vMag
Date/Time June 25, 2008 – 10:20 PM MST (June 26, 2008 – 05:20 UT)
Observing Loc. Flagstaff, AZ – Home
Instrument Orion SkyQuest XT8 (203 mm dia./1200 mm F/L)
Eyepieces/Mag. 10 mm Sirius Plössl (120X)
Conditions Clear, calm
Seeing 5/10 Pickering
Transparency ~ Mag 5.5 NELM
*References SEDS; NGCIC.org

Hickson 70

Hickson 70

Hickson 70
Sketch and Commentary by Bill Ferris
Move cursor over image to see labels.

Hickson 70: Galaxy Cluster (Canes Venatici)
RA: 14h 04.2m / DEC: +33º 20′.3
Instrument: 18-inch Obsession

Hickson 70 resides in far eastern Canes Venatici. The magnificent M3 can be found just 7 degrees to the southwest. But this cluster presents more challenging fare. My sketch combines 199X and 272X views in the 18-inch Obsession. Seven member galaxies in this tightly-packed cluster are visible. Hickson 70A is cataloged as UGC 8990 (=MCG +06-31-59, PGC 50139) and is often misidentified as IC 4371. The 16.1(B) magnitude galaxy resides at 14 hrs., 04 min., 10 sec,; +33 deg., 20.3 minutes and is nearly centered in my sketch. It features a stellar core and covers a 0′.7 by 0′.3 area. Hickson 70D (=IC 4370, MCG +06-31-60) appears as a tiny, 16th magnitude smudge along the northern edge of Hickson 70A. About 2′ to the south, Hickson 70B (=IC 4371, MCG +06-31-61, PGC 50140) displays a stellar core embedded within a 0′.5 by 0′.3 oval glow. 11.0 magnitude SAO 63918 simmers another 2′.3 to the south. The thin sliver of light 2′ to the east of Hickson 70B is MCG +06-31-064. This 16.2(B) magnitude galaxy covers a 0′.5 by 0′.2 area and is aligned northeast to southwest. Three galaxies are grouped to the southwest of Hickson 70A. These include 16.2(B) magnitude Hickson 70E (=IC 4369, MCG +06-31-58, PGC 50134), 17.3(B) magnitude Hickson 70F (=MCG +06-31-57, PGC 50133), and 17.4 magnitude 2MASX J14040011+3319540. Hicksons 70E and 70F are very close to each other and just 1′.3 southwest of Hickson 70A. High magnification was needed to consistently separate the two.

Hickson 44

NGC 3190

Hickson 44
Sketch and Commentary by Kiminori Ikebe

NGC 3185 Leo galaxy
NGC 3187 Leo galaxy
NGC 3190 Leo galaxy
NGC 3193 Leo galaxy
HCG44

1997.01.12 01:27
32cm at 110x

A fine group of four different-type galaxies.
NGC 3185: The largest of the group, but faint and diffuse. Elongated. A fainter halo appears to envelop the galaxy, but not confirmed.
NGC 3187: Barely detectable. A long, narrow shape is barely discerned.
NGC 3190: A sharp, long, spindle-shape. The brightest of the group. A stellar nucleus and a small central condensation.
NGC 3193: Small and round. A dull glow of a stellar nucleus and very weak central condensation.