NGC 6552 is a Barred Spiral Galaxy in the Draco constellation. NGC 6552 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Given its B magnitude of 14.6, NGC 6552 is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.

< NGC List NGC 6552. NGC 6552 is a barred spiral galaxy located in the constellation of Draco. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 6552:

From Redmond , NGC6552 is visible all night because it is circumpolar. It will be highest in the sky shortly before dawn, when it will be lost to twilight at around 05:53, 68° above your northern horizon. At dusk, it will become visible at around 20:35 (PDT), 25° above your northern horizon.

2022年6月16日 · This portion of the MIRI MRS wavelength range shows engineering calibration data obtained of the Seyfert galaxy NGC 6552 (red line) in the constellation Draco. The strong emission feature is due to molecular hydrogen, with an additional weaker feature nearby.

最近，天文学家使用詹姆斯·韦伯太空望远镜（jwst）的中红外仪器（miri）观察了一个名为ngc 6552的星系。 通过对这个星系的观测，他们发现了一个核高电离喷流，这是首次在这个星系中观测到。

This file was last modified on Friday, 09-Jul-1999 12:04:55 EDT Curator: Michael Arida (SP Sys); [email protected] HEASARC Guest Observer Facility

NGC 6552 este o astronomical radio source ⁠(d) situată în constelația Dragonul. [3] [4] [5] A fost descoperită în 6 octombrie 1866 de către Heinrich Louis d'Arrest. [6]

NGC 6552 est une galaxie spirale barrée située dans la constellation du Dragon. Sa vitesse par rapport au fond diffus cosmologique est de 7 870 ± 25 km/s, ce qui correspond à une distance de Hubble de 116,1 ± 8,1 Mpc (∼379 millions d' al) 1. NGC 6552 a été découverte par l'astronome prussien Heinrich d'Arrest en 1866.

IC 4677 ist der helle Teil des Halos rechts neben dem Zentrum des PNs, NGC 6552 ist die Galaxie am linken Bildrand (Typ SBbc, Abstand ~ 350 MLy / 100 Mpc). CCDSharp und DDP wurden benutzt.

NGC 6552 is an active galactic nucleus (AGN) at a redshift of 0.0266 (DL = 120 Mpc) classified as a Seyfert 2 nucleus in the optical and Compton-thick AGN in the X-ray. Aims. This work exemplifies and demonstrates the MRS capabilities to study the mid-infrared (mid-IR) spectra and characterise the physical conditions and kinematics of the ...