
NGC 6837 - Open Cluster in Aquila - TheSkyLive.com
NGC 6837 is a Open Cluster in the Aquila constellation. NGC 6837 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. The image below is a photograph of NGC 6837 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel.
NGC6837 (Open cluster) - In-The-Sky.org
From Virginia Beach , NGC6837 is visible in the dawn sky, rising at 02:56 (EDT) and reaching an altitude of 38° above the eastern horizon before fading from view as dawn breaks at around 06:15. All times shown in Virginia Beach local time.
NGC 6837 GalaxyFacts - Universe Guide
NGC 6837 is a Spiral Galaxy located in the constellation of Aquila in the equatorial region. NGC 6837 is called NGC 6837 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to …
NGC 6837 - Wikipedia
NGC 6837 je otvoreno zvjezdano jato i nalazi se u sazviježđu Orao. Prvo otkriće je napravio John Frederick William Herschel 4. septembra 1784. godine. [ 2 ][ 4 ][ 5 ]
M71 - 维基百科,自由的百科全书
M71 (也稱為 梅西耶71 或 NGC 6838)是一個位於 北天 小 星座 天箭座 的 球狀星團。 它是由 Philippe Loys de Chéseaux (英语:Philippe Loys de Chéseaux) 於1745年發現的,並於1780年被 查爾斯·梅西耶 收錄其非 彗星 天體目錄中。
Revised NGC Data for NGC 6837 - Students for the Exploration …
Note: (*) Dreyer's Object Revised NGC and IC Catalog NGC/IC data for NGC 6837 Back to NGC 6837 page Hartmut Frommert [contact]
NGC 6837 | open cluster in Aquila | NGC List | GO ASTRONOMY
NGC 6837 is a open cluster located in the constellation Aquila. Some key stats include: ... Right Ascension units = HH:MM:SS.SS Declination units = DD:MM:SS.SS PN = planetary nebula
Open cluster NGC 6837 - Open Cluster in Aquila Constellation
Pictures, altitude charts, data sheet and sky map for NGC 6837 - Open cluster in Aquila Constellation
NGC 6837 - Wikidata
Global survey of star clusters in the Milky Way. III. 139 new open clusters at high Galactic latitudesgalaxy
NGC 6837 - Cúmulo / Objeto Múltiple - SKY-MAP
The IR/H I relation is employed to derive relative distances to 10nearby galaxy clusters. A problem originally identified by van den Bergh (1981), that the surface brightnesses of galaxies in the higher redshiftclusters are in the mean found to be lower than in nearby clusters atfixed velocity width, is discussed. The extent to which this effect isaccounted for by galaxy diameter errors is ...