NGC 4699

NGC 4699 is a very tightly wound spiral galaxy with the hint of a bar-like structure in its nucleus. At a distance of 60 million light years away, it resides at the outskirts of the Virgo Cluster of galaxies. Though small, this galaxy is quite bright and makes a good target for amateur CCD imagers. In the past, this galaxy has had a number of bright supernovae explosions and so it makes a good galaxy to keep on eye on for future activity. NGC 4699 is similar in structure to galaxies such as NGC 2775, NGC 2841 and NGC 488.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.

Créditos:

KPNO/NOIRLab/NSF/AURA/Michael Vogel and Robert Mitsch/Adam Block

About the Image

Id:noao-n4699vogel
Tipo:Observation
Release date:4 de Marzo de 2014 a las 12:31
Size:1074 x 1410 px

Sobre el Objeto

Nombre:NGC 4699
Constellation:Virgo
Categoría:Galaxies

Formatos de Imágenes

Large JPEGLarge JPEG
241,2 KB
Screensize JPEGScreensize JPEG
154,6 KB

Zoomable


Fondos de Pantalla

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165,9 KB
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232,4 KB
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304,4 KB
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1,9 MB

Coordenadas

ObjectValue
Posición (AR):12 49 2.03
Posición (Dec):-8° 40' 21.44"
Campo visual:8.13 x 10.68 arcminutes
Orientación:North is 149.9° right of vertical


Colores y Filtros

BandaLongitud de OndaTelescopio
Optical
B
438 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
G
475 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
R
625 nmVisitor Center 0.5-meter Telescope
Other CCD
Optical
Broad Band
555 nmVisitor Center 0.5-meter Telescope
Other CCD