`star-formation` Related Article Results

The NGC 1569 Galaxy is an irregular dwarf galaxy located in the nearby cosmic environment of the Milky Way, characterized by intense star formation activity. Situated at a distance of approximately 11 million light years (3.36 Mpc), this galaxy is observed in the constellation Camelopardalis (Giraffe). NGC 1569 is particularly notable for its recent period of intense star formation, known as a starburst, which has lasted over the past few hundred million years. In this regard, it serves as a cri

NGC 4622 Galaxy is a spiral galaxy located in the constellation Centaurus. It has gained a notable place in astronomical literature due to its unusual characteristics regarding the direction of its spiral arms. First cataloged in the 19th century this galaxy has been studied in detail using modern observational tools such as the Hubble Space Telescope. Observational History and the Leading Arm Phenomenon NGC 4622 was first observed in the 1830s by James Dunlop and later cataloged by John Hersche

The NGC 6240 Galaxy is a merging galaxy pair located approximately 400 million light-years away in the direction of the Scorpius constellation. This galaxy pair consists of two large galaxies in the process of merging and attracts attention for both its structural and dynamic properties as observed. NGC 6240 serves as a critical example in studies due to its high-energy radiation sources and complex gas dynamics. Structural and Dynamic Properties NGC 6240 is a system with two distinct nuclei, in

NGC 1569 is an irregular dwarf galaxy with high star formation activity, located in the nearby cosmic neighborhood of the Milky Way Galaxy. Situated approximately 11 million light-years (3.36 Mpc) away, this galaxy is observed in the constellation Camelopardalis. NGC 1569 stands out for its intense starburst phase that occurred within the last few hundred million years. In this regard, it serves as a critical example for observational and theoretical studies on the galactic-scale effects of star

NGC 3628 Galaxy is an unbarred spiral galaxy located in the constellation Leo, observed edge-on from Earth. Although this galaxy is often referred to in astronomical sources as the "Hamburger Galaxy," such nicknames are not used in academic contexts. NGC 3628 is a member of the galaxy group known as the "Leo Triplet", along with Messier 65 (M65) and Messier 66 (M66). This structure provides an important area of study, particularly for observing interactive galaxy dynamics and external gravitatio

NGC 4650A Galaxy is a galaxy located in the direction of the Cetus constellation and classified in astronomical literature as a "polar ring galaxy." First discovered in the mid-20th century, this galaxy attracts attention due to its ring structure, which is positioned at a right angle to the main body. NGC 4650A is one of the best-studied and exemplary celestial objects among polar ring galaxies. NGC 4650A Galaxy (NASA) " image-element-format="right" image-source="https://cdn.t3pedia.org/media/u

NGC 6240 Galaxy is a pair of colliding galaxies located approximately 400 million light-years away in the direction of the Scorpius constellation. This galaxy pair consists of two large galaxies in the process of merging and stands out in observations due to its structural and dynamic characteristics. NGC 6240, in particular, serves as a critical example in research due to its high-energy radiation sources and complex gas dynamics. NGC 6240 Galaxy (NASA) " image-element-format="right" image-sour

NGC 7318 A Galaxy is one of the prominent members of the galaxy group known as Stephan’s Quintet. This group is one of the regions of special interest for astronomers to study dynamic interactions between galaxies, and it is frequently observed in detail, particularly by NASA’s Hubble Space Telescope and James Webb Space Telescope. Due to its close proximity within the group, NGC 7318 A is in strong gravitational interaction with surrounding galaxies; this situation causes noticeable distortions

The Trifid Nebula is a complex type of nebula located in the constellation Sagittarius in the sky, exhibiting both emission and reflection nebula characteristics. Also known as Messier 20 (M20), this structure is located approximately 5,000 light-years away and is about 40 light-years wide. The name "Trifid" comes from the dark dust lanes passing through the center of the nebula, dividing it into three main regions. Structure and Type The Trifid Nebula stands out for housing three different type

Andromeda Galaxy (M31) is the closest spiral galaxy to the Milky Way and is located approximately 2.5 million light-years away. As the farthest celestial object visible to the naked eye, Andromeda holds great importance for astronomers. Providing critical information about galaxy formation and evolution in the universe, Andromeda is at the center of many scientific studies. Discovery and History Observations of the Andromeda Galaxy date back to ancient times. In 964, the Persian astronomer Abd a