Dragonfish Nebula

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title: "Dragonfish Nebula" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["emission-nebulae", "crux"] description: "Emission nebula and star-forming region in the constellation Crux" topic_path: "general/emission-nebulae" source: "https://en.wikipedia.org/wiki/Dragonfish_Nebula" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

::summary Emission nebula and star-forming region in the constellation Crux ::

::data[format=table title="Infobox nebula"]

Field	Value
name	Dragonfish Nebula
image	Dragonfish600.jpg
caption	Infrared image from the Spitzer Space Telescope
credit	NASA/JPL-Caltech/Univ. of Toronto
type	emission
type2
epoch	J2000
ra
dec
dist_ly
dist_pc
appdia
constellation	Crux
dimensions	130′
names	GAL 298.4-00.4
::

|name = Dragonfish Nebula |image = Dragonfish600.jpg |caption = Infrared image from the Spitzer Space Telescope |credit = NASA/JPL-Caltech/Univ. of Toronto |type = emission |type2 = |epoch = J2000 |subtype = |class = |ra = |dec = |dist_ly = |dist_pc = |dist_z = |appmag_v = |appdia = |size_v = |constellation = Crux |radius_ly = |radius_pc = |dimensions = 130′ |absmag_v = |notes = |names = GAL 298.4-00.4 The Dragonfish Nebula, as it is known for its appearance on infrared images, is a massive emission nebula and star-forming region 30,000 light-years from the Sun in the direction of the constellation Crux, the Southern Cross.

The Dragonfish Nebula gets its name from a giant toothy fish known as the deep-sea dragonfish. The giant stars in this nebula blow a bubble in the surrounding gas. This bubble is over 100 light-years long and forms the mouth of the dragonfish. The two largest and luminous stars, which form its eyes, are said to be newly formed stars. The stars heat up the surrounding gas, giving off infrared light. The Dragonfish Nebula contains some of the most massive stars in the Milky Way galaxy.

This nebula was first discovered in 2010 by Mubdi Rahman and Norman Murray from the University of Toronto. They discovered a cloud of ionized gas which led them to suspect that it was formed from the radiation of nearby stars. Since then more than four hundred stars have been found and there is reason to believe that many smaller stars are hiding in the cluster. The ionized gas around this cluster produces more microwaves than most clusters in our galaxy, making the Dragonfish Nebula the brightest and most massive cluster discovered so far.

Characteristics

Due to its distance and location, it is totally invisible in visible light because the interstellar dust absorbs and reddens its light, hiding it. So in order to study it, wavelengths that are not affected, like infrared, are required.

Research done with the help of the Spitzer Space Telescope has shown this object has a size of 450 light-years, having a large cavity with a diameter of 100 light-years that was created by the strong stellar winds of the young and massive stars inside it.

As of 2011, approximately 400 stars of spectral types O and B have been identified within the nebula. |last1=Rahman |first1=M. |last2=Matzner |first2=C. |last3=Moon |first3=Dae-Sik |year=2011 |title= A Candidate for the Most Luminous OB Association in the Galaxy |journal=The Astrophysical Journal Letters |volume=728 |issue=2 |pages=L37 |id=article ID:L37 |bibcode=2011ApJ...728L..37R |doi=10.1088/2041-8205/728/2/L37 |arxiv = 1101.3323 |s2cid=118599139 }} Subsequent studies have confirmed not only at least 15 O-type stars but also 3 luminous blue variable/Wolf–Rayet star candidates. They also have calculated the total mass of the stars associated with the Dragonfish nebula as 105 solar masses, a mass only comparable with that of the super star cluster Westerlund 1, the most massive OB association and the brightest nebula known in our galaxy. |last1=Rahman |first1=M. |last2=Matzner |first2=C. D. |last3=Moon |first3=Dae-Sik |year=2011 |title=Spectroscopic Confirmation of the Dragonfish Association: The Galaxy's Most Luminous OB Association |journal=The Astrophysical Journal Letters |volume=743 |issue=2 |pages=L28 |id=article ID:L28 |bibcode=2011ApJ...743L..28R |doi=10.1088/2041-8205/743/2/L28 |arxiv = 1111.3362 |s2cid=118410152 }}

References

References

1. "NAME Dragonfish Nebula".
2. "Dragonfish Coming at You in Infrared".
3. "Dragonfish Coming at You in Infrared".
4. (January 2011). "Dragonfish nebula conceals giant star cluster". New Scientist.

::callout[type=info title="Wikipedia Source"] This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page. ::