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I B Thompson

Showing results (1-10 of 6) with videos related to

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Nature|November 26, 2010
The dynamical mass of a classical Cepheid variable star in an eclipsing binary systemG Pietrzyński, I B Thompson, W Gieren, et al.
Nature|April 7, 2012
RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary systemG Pietrzyński, I B Thompson, W Gieren, et al.
Nature|March 15, 2019
A distance to the Large Magellanic Cloud that is precise to one per centG Pietrzyński, D Graczyk, A Gallenne, et al.
Science (New York, N.Y.)|August 13, 2011
Circumstellar material in type Ia supernovae via sodium absorption featuresA Sternberg, A Gal-Yam, J D Simon, et al.
Nature|March 8, 2013
An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per centG Pietrzyński, D Graczyk, W Gieren, et al.
Science (New York, N.Y.)|January 28, 2016
Astronomy. ASASSN-15lh: A highly super-luminous supernovaSubo Dong, B J Shappee, J L Prieto, et al.
Pageof 1

Showing results (1-10 of 6) with videos related to

Sort By:
Pageof 1
Nature|November 26, 2010
The dynamical mass of a classical Cepheid variable star in an eclipsing binary systemG Pietrzyński, I B Thompson, W Gieren, et al.
Nature|April 7, 2012
RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary systemG Pietrzyński, I B Thompson, W Gieren, et al.
Nature|March 15, 2019
A distance to the Large Magellanic Cloud that is precise to one per centG Pietrzyński, D Graczyk, A Gallenne, et al.
Science (New York, N.Y.)|August 13, 2011
Circumstellar material in type Ia supernovae via sodium absorption featuresA Sternberg, A Gal-Yam, J D Simon, et al.
Nature|March 8, 2013
An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per centG Pietrzyński, D Graczyk, W Gieren, et al.
Science (New York, N.Y.)|January 28, 2016
Astronomy. ASASSN-15lh: A highly super-luminous supernovaSubo Dong, B J Shappee, J L Prieto, et al.
Pageof 1