An analysis of STIS HST UV spectra of M 33 early B supergiants
Blue Luminous Stars in Nearby Galaxies: Quantitative Spectral Analysis of M33 B-Type Supergiant Stars
Chemical abundances and winds of massive stars in M31: a B-type supergiant and a WC star in OB 10
Dust Extinction Law in Nearby Star-resolved Galaxies. I. M31 Traced by Supergiants
New Ultraviolet Extinction Curves for Interstellar Dust in M31
Space Telescope Imaging Spectrograph Ultraviolet Spectroscopy of Early B Supergiants in M31
Stellar population of the superbubble N 206 in the LMC. II. Parameters of the OB and WR stars, and the total massive star feedback
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1999-01-04T01:23:10Z/2000-12-11T15:30:27Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Kudritzki et al., 2006, 'The Wind-momentum Luminosity Relationship for M31 and M33 B-supergiants', 1.0, European Space Agency, https://doi.org/10.5270/esa-5d30ha0