M5 (also known as NGC 5904 or the Rose Cluster) is a globular cluster in the constellation Serpens. It was discovered by Gottfried Kirch in 1702. M5 is...

X-ray astronomy is an observational branch of astronomy which deals with the study of X-ray observation and detection from astronomical objects. X-radiation...

2024-04-28. "IC 4537". spider.seds.org. Retrieved 2024-04-28. Pommier, Rod. "M5 AND GALAXY IC 4537 IN SERPENS". Sky & Telescope. Retrieved 2024-04-28....

researchers picked different limits, for example K8–M5 or "later than K5". Dwarf M star, abbreviated dM, was also used, but sometimes it also included stars...

pair of stars separated by only 0.066", about 10 AU, both with spectral type M5.5. Finally, the variable primary star was found to have a faint companion...

as an X1. M-class flares are a tenth the size of X-class flares with the same numeric suffix. An X2 is four times more powerful than an M5 flare. X-class...

Richards, A. M. S; Baudry, A; Maercker, M; Decin, L; Humphreys, E. M (2015). "ALMA observations of TiO2 around VY Canis Majoris". Astronomy and Astrophysics...

K2-415 is an M5 red dwarf star located 72 light-years from Earth. K2-415 has a mass that is 16% of the mass of the Sun. The star has one known planet orbiting...

Hertzsprung–Russell diagram and is of spectral class M5.5. The M5.5 class means that it falls in the low-mass end of M-type dwarf stars, with its hue shifted toward...

Observations - Variables M5, 1896 | HOLLIS for". Project Phaedra: Preserving Harvard's Early Data and Research in Astronomy Harvard College Observatory...