NGC 2149 is a Reflection Nebula in the Monoceros constellation. NGC 2149 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year.

NGC 2149 is a reflection nebula, 1300 light years away in Monoceros. It is rarely imaged, have not seen many images of it anywhere. The field of view has some fascinating checkerboard dark nebulosity...

At image center is the reflection nebula NGC 2149, located 1300 light years away. This nebula spans 3 arc-minutes in our apparent view, which corresponds to a diameter of just over 1 light year. The nebula is accentuated by a superimposed dark nebula Dobashi 5004, just above and left of the brightest portion of NGC 2149.

NGC 2149 是 麒麟座 的一個 星系。 维基共享资源 上的相關多媒體資源： NGC 2149 NED – NGC 2149 SEDS – NGC 2149 SIMBAD – NGC 2149 VizieR – NGC 2149

NGC 2149 is a somewhat unknown reflection nebula in the southwest corner of Monoceros. Just to its west is smaller, dimmer and less defined vdB 66 around a 10th magnitude star. Steven …

2022年11月9日 · Situated 1300 light years away in Monoceros, NGC 2149 is a reflection nebula. The nebula appears to be a giant expanding ring between the high longitude end of the Orion A (molecular) Cloud and the Mon R2 Cloud. In most projections, these clouds appear to …

NGC2149 is a small reflection nebula located in the southwest corner of Monoceros. You can find it approximately 4 degrees due east of κ Orionis (Saiph). Although its size is only about 3 arc …

2022年11月27日 · NGC 2149 is a relatively small reflection nebula 1300 light years away sitting in the midst of a massive cloud of cosmic dust. It spans approximately 1 light year and is around 3’ in the field of view.

NGC 2149 是麒麟座的一个反射星云。

Related articles Infrared Nebulae around Young Stellar ObjectsWe present a K-band atlas of 106 reflection nebulae, 41 of which are newdiscoveries. We observed these nebulae with the University of Hawaii 2.2m telescope in the course of an imaging survey of 197 objects that wereselected as nearby young Class I sources. K-band images andflux-calibrated surface brightness contour plots of each ...