A New Method for the Assessment of Age and Age Spread of Pre-main-sequence Stars in Young Stellar Associations of the Magellanic Clouds
Discovery of the Pre-Main-Sequence Population of the Stellar Association LH 95 in the Large Magellanic Cloud with Hubble Space Telescope Advanced Camera for Surveys Observations
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. VI. The Case of LH 95 in the Large Magellanic Cloud
The Complete Initial Mass Function Down to the Subsolar Regime in the Large Magellanic Cloud with Hubble Space Telescope ACS Observations
The impact of satellite trails on Hubble Space Telescope observations
The massive stellar population in the young association LH 95 in the Large Magellanic Cloud
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC2
Temporal Coverage
2006-03-02T20:53:03Z/2006-03-07T19:35:05Z
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, Gouliermis et al., 2007, 'Star Formation in the LMC - The complete IMF of a Stellar Association', 1.0, European Space Agency, https://doi.org/10.5270/esa-u8jdq3x