A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds, Walborn, Nolan R.,Morrell, Nidia I.,Howarth, Ian D., The Astrophysical Journal, 608, 2004-06-01 00:00:00, 2004ApJ...608.1028W||Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data, Welty, Daniel E.,Xue, Rui,Wong, Tony, The Astrophysical Journal, 745, 2012-02-01 00:00:00, 2012ApJ...745..173W||Nitrogen line spectroscopy in O-stars. III. The earliest O-stars, Rivero González, J. G.,Puls, J.,Massey, P., Astronomy and Astrophysics, 543, 2012-07-01 00:00:00, 2012A&A...543A..95R||The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. I. A Sample of 20 Stars in the Magellanic Clouds, Massey, Philip,Bresolin, Fabio,Kudritzki, Rolf P., The Astrophysical Journal, 608, 2004-06-01 00:00:00, 2004ApJ...608.1001M||The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. II. Analysis of 20 More Magellanic Cloud Stars and Results from the Complete Sample, Massey, Philip,Puls, Joachim,Pauldrach, A. W. A., The Astrophysical Journal, 627, 2005-07-01 00:00:00, 2005ApJ...627..477M||The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. III. More Results From the Magellanic Clouds, Massey, Philip,Zangari, Amanda M.,Morrell, Nidia I., The Astrophysical Journal, 692, 2009-02-01 00:00:00, 2009ApJ...692..618M||The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters, Crowther, Paul A.,Caballero-Nieves, S. M.,Bostroem, K. A., Monthly Notices of the Royal Astronomical Society, 458, 2016-05-01 00:00:00, 2016MNRAS.458..624C||The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence, Bestenlehner, J. M.,Gräfener, G.,Vink, J.... S., Astronomy and Astrophysics, 570, 2014-10-01 00:00:00, 2014A&A...570A..38B||The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution, Shenar, T.,Sablowski, D. P.,Hainich, R., Astronomy and Astrophysics, 627, 2019-07-01 00:00:00, 2019A&A...627A.151S||The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class, Hainich, R.,Rühling, U.,Todt, H., Astronomy and Astrophysics, 565, 2014-05-01 00:00:00, 2014A&A...565A..27H
Instrument
STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2002-05-30T21:55:17Z/2003-08-05T17:35:56Z
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, 2007, The Physical Parameters Of The Hottest, Most Luminous Stars As A Function Of Metallicity, 1.0, European Space Agency, https://doi.org/10.5270/esa-nel8roh
