A Luminous X-Ray Flare from the Nucleus of the Dormant Bulgeless Spiral Galaxy NGC 247
Nature of the Soft ULX in NGC 247: Super-Eddington Outflow and Transition between the Supersoft and Soft Ultraluminous Regimes
New luminous blue variable candidates in the NGC 247 galaxy
Search for LBVs in the Local Volume galaxies: study of four stars in NGC 4449
XMM-Newton campaign on the ultraluminous X-ray source NGC 247 ULX-1: outflows
Instrument
ACS, ACS/SBC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2014-06-30T10:18:30Z/2014-06-30T12:39:28Z
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, Feng comma Hua, 2015, 'Multiwavelength Test For A Standard Accretion Disk Around An Intermediate Mass Black Hole Candidate', 1.0, European Space Agency, https://doi.org/10.5270/esa-g9mz3ai