NGC 5676

{{Infobox Galaxy

| name = NGC 5676

| image = 250px

| alt = NGC 5676

| caption = SDSS image of NGC 5676

| epoch = J2000

| constellation name = Boötes{{cite book

| editor=R. W. Sinnott

| title= The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer

| date=1988

| publisher=Sky Publishing Corporation and Cambridge University Press

| isbn=978-0-933346-51-2}}

| ra = {{RA|14|32|46.8}}{{cite web

| title=NASA/IPAC Extragalactic Database

| work=Results for NGC 5676

| url=http://nedwww.ipac.caltech.edu/

| access-date=2007-07-13}}

| dec = {{DEC|+49|27|28}}

| z = 2114 ± 5 km/s

| dist_ly =100 Mly
(30.8 Mpc)

| type = SA(rs)bc

| appmag_v = 12.3

| size_v = 4.0{{prime}} × 1.1{{prime}}

| notes = Paired with NGC 5660.

| names = UGC 9366, PGC 51978, MCG+08-26-043, H I-189, h 1842, GC 3935, CGCG 247.042, CGCG 248.003, KUG 1431+496, LGG 384-005

}}

NGC 5676 is an unbarred spiral galaxy in the constellation Boötes.

Disk

This spiral galaxy is notably asymmetric. The spiral arms on the south side of the galaxy are chaotic in appearance, whereas the spiral arms on the north side of the galaxy are very well-defined. Also, the spiral arms on the south side of the disk extend twice as far from the galaxy's nucleus as the spiral arms on the north side.{{cite book

| author=A. Sandage

| author2=J. Bedke

| date=1994

| title=Carnegie Atlas of Galaxies

| publisher=Carnegie Institution of Washington

| location=Washington, D.C.

| isbn=978-0-87279-667-6}} Because of the fragmentary appearance of some of the spiral arms, this galaxy is classified as a flocculent galaxy.{{cite journal

| author=D. M. Elmegreen|author-link1=Debra Elmegreen

| author2=B. G. Elmegreen|author-link2=Bruce Elmegreen

| title=Arm classifications for spiral galaxies

| journal=Astrophysical Journal

| date=1987

| volume=314

| pages=3–9

| bibcode=1987ApJ...314....3E

| doi=10.1086/165034}}

Star formation

The north part of the disk also contains what appears to be a very intense region of star formation.{{cite journal

| author= G. J. Bendo

| author2= R. D. Joseph

| title=Nuclear Stellar Populations in the Infrared Space Observatory Atlas of Bright Spiral Galaxies

| journal=Astronomical Journal

| date=2004

| volume=127

| issue= 6

| pages=3338–3360

| bibcode=2004AJ....127.3338B

| doi=10.1086/420712|arxiv = astro-ph/0403133 | s2cid= 14169689

}} Unusually, the star formation within this region appears to be more intense than the star formation in the galaxy's nucleus, and it is the brightest infrared source within the disk.{{cite journal

| author=G. J. Bendo

| display-authors=4

| author2=R. D. Joseph

| author3=M. Wells

| author4=P. Gallais

| author5= M. Haas

| author6= A. M. Heras

| author7= U. Klaas

| author8= R. J. Laureijs

| author9= K. Leech

| author10= D. Lemke

| author11= L. Metcalfe

| author12= M. Rowan-Robinson

| author13= B. Schulz

| author14= C. Telesco

| title=An Infrared Space Observatory Atlas of Bright Spiral Galaxies

| journal=Astronomical Journal

| date=2002

| volume=123

| issue=6

| pages=3067–3107

| bibcode=2002AJ....123.3067B

| doi=10.1086/340083| doi-access=free

}}

References

External links

[http://www.freewebs.com/ebenson/ngc5676.htm www.freewebs.com/]
[http://aladin.u-strasbg.fr/AladinPreview?-c=14+32+47.18%2B49+27+28.6&ident=NGC++5676&submit=Aladin+previewer Image NGC 5676]
{{WikiSky}}

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! colspan="1" | Database references

bgcolor="#FFFAFA"

| Simbad

[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+5676&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id data]