Celestial Atlas
(NGC 4350 - 4399) <—     NGC Objects: NGC 4400 - 4449     —> (NGC 4450 - 4499)
Click here for Introductory Material
QuickLinks:
4400, 4401, 4402, 4403, 4404, 4405, 4406, 4407, 4408, 4409, 4410, 4411, 4412, 4413, 4414, 4415, 4416,
4417, 4418, 4419, 4420, 4421, 4422, 4423, 4424, 4425, 4426, 4427, 4428, 4429, 4430, 4431, 4432, 4433,
4434, 4435, 4436, 4437, 4438, 4439, 4440, 4441, 4442, 4443, 4444, 4445, 4446, 4447, 4448, 4449

Page last updated Jul 26, 2011
WORKING: Add positions/physical data (per Steinicke)

NGC 4400
Discovered (Apr 13, 1850) by
George Stoney
An emission region in Canes Venatici (RA 12 25 55.9, Dec +33 30 57)

Part of NGC 4395. Dreyer lists NGC 4400 as reported by Stoney's employer, William Parsons, but notes that most of his discoveries were actually made by his assistants.

SDSS image of NGC 4400 and 4401
Above, a 2.4 arcmin wide closeup of NGC 4400 and 4401
Below, a labeled image of NGC 4395 showing the HII regions listed as NGC 4399, 4400, and 4401
SDSS image of NGC 4395, showing emission regions NGC 4399, 4400 and 4401

NGC 4401
Discovered (Jul 29, 1827) by
John Herschel
An emission region in Canes Venatici (RA 12 25 57.9, Dec +33 31 38)

Part of galaxy NGC 4395, and close to NGC 4400, which see for images.


NGC 4402 (= PGC 40644)
Discovered (Mar 5, 1862) by
Arthur von Auwers
A 12th-magnitude edge-on spiral galaxy (type Sb) in Virgo (RA 12 26 07.8, Dec +13 06 47)

NGC 4402's recessional velocity of 230 km/sec is too small to be a reliable indicator of distance, as peculiar (non-Hubble expansion) velocities could be a substantial portion of the value; and in fact the 10 million light years distance corresponding to its velocity is far smaller than redshift-independent distance estimates of about 50 million light years. Using the more likely distance of 50 million light years, NGC 4402's apparent size of 3.9 by 1.1 arcmins suggests that it is about 55 thousand light years across.

SDSS image of NGC 4402
Above, a 4 arcmin wide closeup of NGC 4402
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region around NGC 4402

NGC 4403
Discovered (Mar 20, 1789) by
William Herschel


NGC 4404
Discovered (Mar 20, 1789) by
William Herschel


NGC 4405 (=
IC 788)
Discovered (Mar 21, 1784) by William Herschel (and later listed as NGC 4405)
Discovered (May 19, 1893) by Stephane Javelle (and later listed as IC 788)


NGC 4406 (=
M86 = PGC 40653), part of Markarian's Chain
Discovered (Mar 18, 1781) by Charles Messier
A 9th-magnitude elliptical galaxy (type E3) in Virgo (RA 12 26 11.5, Dec +12 56 47)

Part of Markarian's Chain, a group of Virgo Cluster galaxies which lie along a smooth curve and have similar radial velocities. (See NGC 4438 for a discussion of a probable "recent" collision or near-miss involving M86 and that galaxy.)

SDSS image of NGC 4406, also known as M86
Above, a 12 arcmin wide closeup of M86
Below, a 24 arcmin wide region centered on the galaxy
SDSS image of region near NGC 4406, also known as M86

NGC 4407 (=
NGC 4413)
Discovered (Apr 17, 1784) by William Herschel (and later listed as NGC 4413)
Discovered (May 4, 1829) by John Herschel (and later listed as NGC 4407)

The second IC notes "Not found by Frost on plate of 4 hours exposure".


NGC 4408 (= PGC 40668)
Discovered (Apr 21, 1865) by
Heinrich d'Arrest
A 14th-magnitude lenticular galaxy (type S0) in Coma Berenices (RA 12 26 17.1, Dec +27 52 16)

Based on a recessional velocity of 7525 km/sec, NGC 4408 is about 350 million light years away. Given that and its apparent size of 0.7 by 0.45 arcmin, it is about 70 thousand light years across.

SDSS image of NGC 4408
Above, a 2.4 arcmin wide closeup of NGC 4408
Below, a 12 arcmin wide region centered on the galaxy; also shown at far left is part of IC 3353
SDSS image of region near NGC 4408

NGC 4409 (=
NGC 4420)
Discovered (Jan 24, 1784) by William Herschel (and later listed as NGC 4420)
Discovered (Feb 23, 1784) by William Herschel (and later listed as NGC 4409)


NGC 4410
Discovered (Jan 18, 1828) by
John Herschel


NGC 4411
Discovered (1881) by
Christian Peters

The second IC notes "I assume that Bigourdan 298, RA 12 19 40, NPD 80 21, very faint, large, 2.5 arcmin, is identical with this".


NGC 4412
Discovered (Feb 23, 1784) by
William Herschel


NGC 4413 (=
NGC 4407)
Discovered (Apr 17, 1784) by William Herschel (and later listed as NGC 4413)
Discovered (May 4, 1829) by John Herschel (and later listed as NGC 4407)


NGC 4414
Discovered (Mar 13, 1785) by
William Herschel


NGC 4415
Discovered (Dec 28, 1785) by
William Herschel


NGC 4416
Discovered (Apr 11, 1825) by
John Herschel


NGC 4417
Discovered (Apr 15, 1784) by
William Herschel


NGC 4418 (=
NGC 4355)
Discovered (Jan 1, 1786) by William Herschel (and later listed as NGC 4418)
Discovered (Feb 5, 1878) by David Todd (and later listed as NGC 4355)


NGC 4419
Discovered (Apr 8, 1784) by
William Herschel


NGC 4420 (=
NGC 4409)
Discovered (Jan 24, 1784) by William Herschel (and later listed as NGC 4420)
Discovered (Feb 23, 1784) by William Herschel (and later listed as NGC 4409)


NGC 4421
Discovered (Mar 21, 1784) by
William Herschel


NGC 4422
Discovered (Apr 25, 1784) by
William Herschel


NGC 4423
Discovered (Apr 13, 1784) by
William Herschel


NGC 4424 (= PGC 40809)
Discovered (Feb 27, 1865) by
Heinrich d'Arrest
A 12th-magnitude barred spiral galaxy (type SB(s)a?) in Virgo (RA 12 27 11.4, Dec +09 25 17)

NGC 4424's recessional velocity of 435 km/sec is too small, in comparison to peculiar (non-Hubble expansion) velocities, to ensure an accurate distance estimate. The distance corresponding to the recessional velocity is 20 million light years, which is less than half the redshift-independent distance estimates of 50 to 55 million light years. Presuming the more likely distance of around 50 million light years, the galaxy's apparent size of 3.6 by 1.8 arcmins would make it about 50 thousand light years across.

SDSS image of NGC 4424
Above, a 4 arcmin wide closeup of NGC 4424
Below, a 12 arcmin region centered on the galaxy
SDSS image of region near NGC 4424

NGC 4425
Discovered (Apr 17, 1784) by
William Herschel


NGC 4426 (=
NGC 4427)
Recorded (Apr 21, 1865) by Heinrich d'Arrest (and later listed as NGC 4426)
Recorded (Apr 22, 1886) by Guillaume Bigourdan (and later listed as NGC 4427)
A pair of stars in Coma Berenices (RA 12 27 10.5, Dec +27 50 22)

The second IC notes (per Max Wolf, list IV) "4426-27 are only 2 stars 36 arcsec apart, north and south".


NGC 4427 (=
NGC 4426)
Recorded (Apr 21, 1865) by Heinrich d'Arrest (and later listed as NGC 4426)
Recorded (Apr 22, 1886) by Guillaume Bigourdan (II-53) (and later listed as NGC 4427)
A pair of stars in Coma Berenices (RA 12 27 10.5, Dec +27 50 22)

The second IC notes (per Max Wolf, list IV) "4426-27 are only 2 stars 36 arcsec apart, north and south".


NGC 4428
Discovered (Mar 16, 1828) by
John Herschel


NGC 4429
Discovered (Mar 15, 1784) by
William Herschel


NGC 4430
Discovered (Apr 13, 1784) by
William Herschel


NGC 4431
Discovered (Apr 17, 1784) by
William Herschel


NGC 4432
Discovered (Mar 22, 1865) by
Albert Marth (240)


NGC 4433
Discovered (Mar 16, 1828) by
John Herschel


NGC 4434
Discovered (Dec 28, 1785) by
William Herschel


NGC 4435 (= PGC 40898; with
NGC 4438, The Eyes = Arp 120)
Part of Markarian's Chain

Discovered (April 8, 1784) by William Herschel
An 11th-magnitude lenticular galaxy (type Sb0?) in Virgo (RA 12 27 40.5, Dec +13 04 47)

Part of Markarian's Chain, a group of Virgo Cluster galaxies which lie along a smooth curve and have similar radial velocities.

SDSS image of NGC 4435
Above, a 2.4 arcmin wide closeup of NGC 4435
Below, a 12 arcmin wide region centered between NGC 4435 and 4438, "The Eyes"
SDSS image of NGC 4435 and 4438, also known as The Eyes

NGC 4436
Discovered (April 17, 1784) by
William Herschel


NGC 4437 (=
NGC 4517)
Discovered (Feb 22, 1784) by William Herschel (and later listed as NGC 4517)
Discovered (Apr 14, 1828) by John Herschel (and later listed as NGC 4437)


NGC 4438 (= PGC 40914; with
NGC 4435, The Eyes = Arp 120)
Part of Markarian's Chain

Discovered (April 8, 1784) by William Herschel
A 10th-magnitude lenticular galaxy in Virgo (RA 12 27 45.6, Dec +13 00 31)

Part of Markarian's Chain, a group of Virgo Cluster galaxies which lie along a smooth curve and have similar radial velocities. The distorted shape of NGC 4438 has been interpreted in various ways; but an NOAO study shows that there is a 400 thousand light year long swath of hydrogen gas stretching between M86 and NGC 4438, suggesting that a high-speed collision (or near-miss) between the two galaxies a few tens of millions of years ago is the cause of the distortion.

SDSS image of NGC 4438
Above, an 8 arcmin wide closeup of NGC 4438; part of NGC 4435 is also shown
Below, a 12 arcmin wide region centered between NGC 4438 and 4435, "The Eyes"
SDSS image of NGC 4435 and 4438, also known as The Eyes
Below, an NOAO image of the pair shows more central detail (Image Credits: Adam Block/NOAO/AURA/NSF)
NOAO image of NGC 4435 and 4438, also known as The Eyes
Below, a "deep" hydrogen emission (Hα) image of the region between M86 and NGC 4438
(Image Credits: Tomer Tal and Jeffrey Kenney/Yale University and NOAO/AURA/NSF)
NOAO image of H-Alpha hydrogen emission in the region between M86 and NGC 4438

NGC 4439
Discovered (April 30, 1826) by
James Dunlop (300)


NGC 4440
Discovered (April 17, 1784) by
William Herschel


NGC 4441
Discovered (Mar 20, 1790) by
William Herschel


NGC 4442
Discovered (April 15, 1784) by
William Herschel


NGC 4443 (=
NGC 4461 = PGC 41111)
Discovered (April 12, 1784) by William Herschel (and later listed as NGC 4461)
Discovered (Apr 13, 1850) by George Stoney (and later listed as NGC 4443)
An 11th-magnitude lenticular galaxy (type SB0/a) in Virgo (RA 12 29 02.9, Dec +13 11 04)

The second IC notes "Not found by Frost on plate of 4 hours exposure". (Part of Markarian's Chain, under its listing as NGC 4461)


NGC 4444
Discovered (Mar 15, 1836) by
John Herschel


NGC 4445 (=
IC 793)
Discovere (Apr 24, 1865) by Heinrich d'Arrest (and later listed as NGC 4445)
Discovered (May 6, 1888) by Lewis Swift (and later listed as IC 793)


NGC 4446
Discovered (Apr 17, 1887) by
Lewis Swift (6-43)


NGC 4447
Discovered (Apr 17, 1887) by
Lewis Swift (6-44)


NGC 4448
Discovered (Apr 11, 1785) by
William Herschel


NGC 4449 (= PGC 40973 = PGC 2236413)
Discovered (Apr 27, 1788) by
William Herschel
A 10th-magnitude dwarf irregular galaxy (type IBm) in Canes Venatici (RA 12 28 11.3, Dec +44 05 42)

Per Dreyer, NGC 4449 (= John Herschel's GC 3002, 1860 RA 12 21 23, NPD 45 08.0) is "very bright, considerably large, much extended, double or bifid (either a double nebula, or a single nebula split into two lobes), well-resolved (clearly consisting of stars), 9th-magnitude star 5 arcmin to east". The position precesses to RA 12 28 13.4, Dec +44 05 30, about 0.6 arcmin southeast of the center of the galaxy, but for such a large and irregular object an insignificant error, so the identification is certain. Based on a recessional velocity of 205 km/sec, NGC 4449 is about 10 million light years away. For such a small distance, peculiar (non-Hubble expansion) velocities can significantly affect the accuracy of the result, but as it happens, the value is in good agree with redshift-independent distance estimates of 10 to 14 million light years. Using the generally presumed distance of 12 million light years and its apparent size of 6.2 by 4.4 arcmin, the galaxy is about 20 thousand light years across. Its structure and size appear similar to the Large Magellanic Cloud, a satellite of our galaxy, but it is not a member of our Local Group, but of the nearby Canes Venatici group of galaxies. Radio imaging indicates that the "dwarf" is embedded in a gaseous halo nearly 200 thousand light years across, or a thousand times the volume of the visible galaxy(!)

SDSS image of NGC 4449
Above, an 8 arcmin "closeup" of NGC 4449
Below, a ground-based view of the galaxy emphasizing its HII regions
(Image Credits: John and Christie Connors/Adam Block/AURA/NSF/NOAO)
NOAO image of NGC 4449
Below, a HST closeup of the galaxy (with North on the right, to show more detail)
(Image Credits: ESA, A. Aloisi (STScI/ESA), and The Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, NASA)
HST image of NGC 4449
Below, an alternate version of the HST image emphasizing its HII regions
(Image Credits: Data - Hubble Legacy Archive, ESA, NASA; Processing - Robert Gendler, Courtney Seligman)
HST image of emission regions in NGC 4449
Below, a 12 arcmin wide region centered on the galaxy (with North on top, as usual)
SDSS image of region near NGC 4449
Celestial Atlas
(NGC 4350 - 4399) <—     NGC Objects: NGC 4400 - 4449     —> (NGC 4450 - 4499)
Click here for Introductory Material