
NGC 1798 - 维基百科,自由的百科全书
NGC 1798,又記作 OCL 410,是 御夫座 的 疏散星团,由 愛德華·巴納德 於1885年發現。 後來 約翰·德雷耳 將其收入原版 天體新總表 (NGC),形容為「一小團恆星,或有星雲狀物」。
Study inspects two old open clusters - Phys.org
2022年7月19日 · Using the San Pedro Martir Observatory and data from ESA's Gaia satellite, astronomers have inspected two old open clusters (OCs) known as NGC 1798 and NGC …
NGC 1798 - Open Cluster in Auriga - TheSkyLive.com
NGC 1798 is a Open Cluster in the Auriga constellation. NGC 1798 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. The …
NGC 1798 — Wikipédia
NGC 1798 est un amas ouvert situé dans la constellation du Cocher. Il a été découvert par l'astronome américain Edward Barnard en 1885. NGC 1798 est à une distance d'environ 3 …
Berkeley 16 - Experienced Deep Sky Imaging - Cloudy Nights
Berkeley 16 (NGC 1798) is a trumpler (https://en.wikipedia..._classification) class II 2 p open cluster located approximately 15,000 light-years away in Auriga. Imaged January 10th, 2022 …
NGC1798 (Open cluster) - In-The-Sky.org
From Virginia Beach , NGC1798 is visible in the evening sky, becoming accessible around 18:32 (EST), 66° above your north-eastern horizon, as dusk fades to darkness. It will then reach its …
A study of the NGC 1193 and NGC 1798 open clusters using CCD …
2022年7月13日 · We present photometric, astrometric, and kinematic studies of the old open star clusters NGC 1193 and NGC 1798. Both of the clusters are investigated by combining data …
UBVI CCD photometry of two old open clusters NGC 1798 and NGC …
1999年1月12日 · We present UBVI CCD photometry of two open clusters NGC 1798 and NGC 2192 which were little studied before. Color-magnitude diagrams of these clusters show …
NGC 1798 - 维基百科,自由的百科全书 - zh.wikipedia.org
NGC 1798,又记作 OCL 410,是 御夫座 的 疏散星团,由 爱德华·巴纳德 于1885年发现。 后来 约翰·德雷耳 将其收入原版 天体新总表 (NGC),形容为“一小团恒星,或有星云状物”。
Radial velocities and metallicities from infrared Ca II triplet ...
2012年7月13日 · Results: We provide the first spectroscopic determinations of radial velocities and metallicities for the open clusters Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266.