Add to ORKGThe MACHO microlensing experiment's time-sampled photometry database contains blue and red lightcurves for nearly 9 million stars in the central bar region of the Large Magellanic Cloud (LMC). We have identified known LMC Planetary Nebulae (PN) in the database and find one, Jacoby 5, to be variable. We additionally present data on the ``parent populations`` of LMC PN, and discuss the star formation history of the LMC bar. 14 refs., 1 fig
We study the Large Magellanic Cloud Papillon Nebula (N 159-5), a conspicuous High Excitation Blob (...
This paper examines, compares and plots optical, near-and mid-infrared (MIR) photometric data for 60...
We present new results of a long-term investigation of the stellar content of the Large and the Smal...
We use the eight year light-curve database from the MACHO (MAssive Compact Halo Objects) project tog...
We present an analysis of the period distribution of about 1800 Cepheids in the LMC, based on data o...
We present a 9 million star color-magnitude diagram (9M CMD) of the Large Magellanic Cloud (LMC) bar...
I present a new analysis of the MACHO Project 5.7 year Large Magellanic Cloud (LMC) microlensing dat...
We report the discovery of eight new R Coronae Borealis (RCB) stars in the Large Magellanic Cloud (L...
The MACHO Project is a microlensing survey that monitors the brightnesses of -60 million stars in th...
Planetary Nebulae (PNs) in the Magellanic Clouds offer the unique opportunity to study both the popu...
Using WFPC2 on board the Hubble Space Telescope, we have created deep color-magnitude diagrams in th...
We present our investigation of pre-main-sequence (PMS) stellar populations in the Large Magellanic ...
The MACHO Project monitors millions of stars in the Large Magellanic Cloud, the Small Magellanic Clo...
We attempt to determine whether the MACHO microlensing source stars are drawn from the average popul...
We present Hubble Space Telescope (HST) WFPC2 photometry of 13 microlensed source stars from the 5.7...
We study the Large Magellanic Cloud Papillon Nebula (N 159-5), a conspicuous High Excitation Blob (...
This paper examines, compares and plots optical, near-and mid-infrared (MIR) photometric data for 60...
We present new results of a long-term investigation of the stellar content of the Large and the Smal...
We use the eight year light-curve database from the MACHO (MAssive Compact Halo Objects) project tog...
We present an analysis of the period distribution of about 1800 Cepheids in the LMC, based on data o...
We present a 9 million star color-magnitude diagram (9M CMD) of the Large Magellanic Cloud (LMC) bar...
I present a new analysis of the MACHO Project 5.7 year Large Magellanic Cloud (LMC) microlensing dat...
We report the discovery of eight new R Coronae Borealis (RCB) stars in the Large Magellanic Cloud (L...
The MACHO Project is a microlensing survey that monitors the brightnesses of -60 million stars in th...
Planetary Nebulae (PNs) in the Magellanic Clouds offer the unique opportunity to study both the popu...
Using WFPC2 on board the Hubble Space Telescope, we have created deep color-magnitude diagrams in th...
We present our investigation of pre-main-sequence (PMS) stellar populations in the Large Magellanic ...
The MACHO Project monitors millions of stars in the Large Magellanic Cloud, the Small Magellanic Clo...
We attempt to determine whether the MACHO microlensing source stars are drawn from the average popul...
We present Hubble Space Telescope (HST) WFPC2 photometry of 13 microlensed source stars from the 5.7...
We study the Large Magellanic Cloud Papillon Nebula (N 159-5), a conspicuous High Excitation Blob (...
This paper examines, compares and plots optical, near-and mid-infrared (MIR) photometric data for 60...
We present new results of a long-term investigation of the stellar content of the Large and the Smal...