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> Pismis 24 star cluster in Scorpius

Pismis 24 star cluster in Scorpius

author: R.Gendler/U.Jorgensen/ K.Harpsoe/J.Skottfelt/ IDA/Novapix

reference: a-aou98-00102

Image Size 300 DPI: 17 * 17 cm

Located near the famous "Cat Paw" nebula (NGC 6334), the Stellar Cluster Pismis 24 lies at the core of NGC 6357. Its stars include some of the most massive stellar behemoths known. One of the brightest stars in the cluster, Pismis 24-1, was thought possibly to be the most massive on record, approaching 300 solar masses, until it was discovered by the Hubble Telescope to be a triple star, with large components exceeding 100 solar masses. Several of the other central stars also exceed 100 solar masses. The nebulosity visible in the image shows the effects of intense radiation which has sculpted the clouds into curious shapes. Massive protostars, invisible to optical telescopes, lie hidden within the gas and dust of the region. Image taken with the ESO/Danish 1.5m telescope at La Silla observatory in Chile.

Keywords for this photo:

ASTRONOMY - BINARY STAR - EMISSION NEBULA - MASSIVE STAR - NEBULA - NGC 6357 - OPEN CLUSTER - PISMIS 24 - PISMIS 24-1 - SCORPIUS - STAR - STAR CLUSTER - YOUNG STAR -