📖

Artikel Tidak Ditemukan

Tidak ada artikel Wikipedia untuk "Wolf Rayet".

DEBUG MODE: Kemungkinan IP VPS Anda diblokir oleh Wikipedia atau ada masalah SSL d VPS.
ALASAN ERROR: RAW BODY (200 OK): {"batchcomplete":"","query":{"searchinfo":{"totalhits":0},"search":[]}}

Cari langsung di Wikipedia ↗

📚 Artikel Terkait di Wikipedia

Wolf–Rayet

Wolf–Rayet (WR) can mean: Wolf–Rayet star, a type of evolved, massive star Wolf–Rayet galaxy, which contains large numbers of Wolf–Rayet stars Wolf–Rayet

Wolf–Rayet nebula

A Wolf–Rayet nebula is a type of nebula created from stellar winds expelled by Wolf–Rayet stars. Wolf–Rayet stars are very hot, highly luminous, and rapidly

List of Wolf–Rayet stars

Wolf–Rayet stars, often abbreviated as WR stars, are a rare heterogeneous set of stars with unusual spectra showing prominent broad emission lines of ionised

Starburst galaxy

distant ULIRGs. Wolf–Rayet galaxies (WR galaxies), galaxies where a large portion of the bright stars are Wolf–Rayet stars. The Wolf–Rayet phase is a relatively

Stellar classification

or nitrogen, or sometimes oxygen. Once included as type O stars, the Wolf–Rayet stars of class W or WR are notable for spectra lacking hydrogen lines

Supernova

atmospheres and evolve to Wolf–Rayet stars before their cores collapse. All Wolf–Rayet stars end their lives from the Wolf–Rayet phase within a million years

List of hottest stars

most luminous stars List of least massive stars List of coolest stars "Wolf-Rayet Star Catalogue". pacrowther.staff.shef.ac.uk. Retrieved 2021-05-28. Sander

Hypergiant

explode as a supernova or completely shed their outer layers to become a Wolf–Rayet star. Stars with an initial mass above about 40 M☉ are simply too luminous