The Pelican Nebula (also known as IC 5070 [1]) is an H II region associated with the North America Nebula in the constellation of Cygnus. The gaseous contortions of this emission nebula bear a resemblance to a pelican, giving rise to its name. [1]

2018年12月31日 · Pelican Nebula (IC 5070) The Pelican Nebula is a star-forming nebula located near the bright Deneb at the tail of the celestial Swan. Named for its resemblance to a pelican, the nebula is associated with the nearby North America Nebula (NGC 7000).

鹈鹕星云（IC 5067和IC 5070）距离约2000光年，借助小型望远镜可以在明亮的天津四的东北方向看到它。 [1] 鹈鹕星云，IC星表编号为IC 5070，因为看起来像一只鹈鹕，所以被命名为鹈鹕星云。

鵜鶘星雲（也就是所知的ic 5070和ic 5067）是在天鵝座與北美洲星雲結合在一起的一個電離氫區。這個發射星雲的型狀與鵜鶘相似，因此得到這個名稱。鵜鶘星雲是在天鵝座靠近天津四，占有很大面積的一個巨大發射星雲，並且被一個充滿暗塵埃的分子雲，與相鄰 ...

2016年11月19日 · Also known as IC 5070, this interstellar cloud of gas and dust is appropriately found just off the "east coast" of the North America Nebula (NGC 7000), another surprisingly familiar looking emission nebula in Cygnus.

The Pelican Nebula is an H II region (emission nebula) in the constellation Cygnus. Cataloged as IC 5070, this nebula lies right next to the North America Nebula. The Pelican Nebula contains an active mix of star formation and evolving gas clouds.

[b]The Pelican Nebula[/b] "...also known as IC 5070 and IC 5067, is an H II region associated with the North America Nebula in the constellation Cygnus. The gaseous contortions of this emission nebula...

2024年11月1日 · The Pelican Nebula (IC 5070) is an H II region associated with the North America Nebula in the Cygnus constellation. Contortions resemble a pelican, giving rise to its name. Located 1,800 light-years from Earth, the nebula spans 30 light-years.

2024年10月1日 · The Pelican carries two catalog designations -- IC 5067 and IC 5070 -- that point to two portions of the nebula. The eastern edge of Lynds 935 carves out the outline of the North America Nebula's (terrestrial) east coast, while its western edge forms the long beak and pointy head of the celestial pelican, listed as IC 5070.

2019年9月26日 · 该星云被正式命名为IC 5070，一个满是黑暗尘埃的分子云将它与较庞大的北美星云相隔。 然而，因为鹈鹕星云是恒星形成和演化气体云的特别活跃的混合体，所以它成为了研究的热点。 这幅特征影像是由三种特定的颜色构建而成，它们分别来自硫、氢和氧发出的辉光，这有助于我们更好地理解那些交互作用。 年轻高能恒星发出的星光正缓慢地将冰冷云气转变为炽热气体，这两种气体之间的推进边界被称为电离前沿，在影像右侧的亮橙色区域内可见。 而一些特 …