Geminga /ɡəˈmɪŋɡə/ is a gamma ray and x-ray pulsar source thought to be a neutron star approximately 250 parsecs (around 800 light-years) from the Sun...

Medusa Nebula is another planetary nebula, some 1,500 light-years distant. Geminga is a neutron star approximately 550 light-years from Earth. Other objects...

2011-11-03. Bignami, G. F.; et al. (September 1983). "An identification for 'Geminga' (2CG 195+04) 1E 0630+178 - A unique object in the error box of the high-energy...

supernovae that exploded within the past ten to twenty million years. Geminga, a pulsar in the constellation Gemini, was once thought to be the remnant...

sky. The Vela supernova remnant is one of the closest known to us. The Geminga pulsar is closer (and also resulted from a supernova), and in 1998 another...

supernova remnant is the neutron star Geminga. However, the last is unlikely given the distance between Geminga and the cluster. Lambda Orionis A, B and...

supernovae are the Vela Supernova Remnant (c. 800 ly, c. 12,000 years ago) and Geminga (c. 550 ly, c. 300,000 years ago). Type Ia supernovae are thought to be...

pulsar planets in the future. The existence of a dust cloud at the pulsar Geminga that may be a precursor to planets has been proposed. There were earlier...

first unidentified pulsar radio emission, she identified the neutron star Geminga. She has developed a multi-wavelength strategy for the identification of...

control section performed in an excellent manner. SAS-2 first detected Geminga, a pulsar believed to be the remnant of a supernova that exploded 300,000...

pulsar Geminga. The accelerated electrons and positrons collide with nearby starlight. The collision boosts the light to much higher energies. Geminga alone...

found several gamma-ray sources, among which a very strong source called Geminga was later identified as a pulsar in proximity. The Compton Gamma Ray Observatory...

radio waves at the 400 MHz and 1400 MHz frequencies. That exception is Geminga, which is radio quiet at frequencies above 100 MHz, but is a strong emitter...

diffuse X-ray emission by molecular clouds. Detection of pulsations from Geminga. Detection of isolated neutron stars. Discovery of X-ray emission from...

the measurements of the pulsed optical emission from PSR B0656+14 and Geminga (Src). JPL · 11450 11451 Aarongolden 1979 QR1 Aaron Golden (born 1969)...

B0540-69 (in the Large Magellanic Cloud) 23 PSR B0656+14 26 PSR B0633+17 (Geminga) 25.5 PSR B1509-58 (*) 25.7 PSR J1023+0038 22 PSR B1055−52 24.9 PSR B1929+10...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...

nebula is an PG 1159 star. Abell Catalog of Planetary Nebulae　　　　　　　　　　　 Geminga, Gemini gamma-ray source Gemini in Chinese astronomy IC 444, reflection...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...

indicated that the increase in flux of positrons from the two nearest pulsars (Geminga and Monogem) is roughly equivalent to the excess originally observed by...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...

enhanced stability in hot thin plasmas 1993 Nature paper with Wan Chen on the Geminga supernova as a cause of the Local Bubble 1997 in Il Nuovo Cimento on the...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...

J060738.65+242953.4 06h 07m 39.08s +24° 29′ 57.5″ 25.4 L9 brown dwarf Geminga 06h 33m 54.15s +17° 46′ 12.9″ pulsar CXOU J061705.3+222127 06h 17m 05.3s...

emission from compact objects including the Crab Nebula, and the discovery of Geminga. The SAS II gamma ray telescope's successful results during the 1970s brought...

discovery of a radio pulsar 102 MHz while observing X-ray radio source Geminga, another radio pulsar discovered as the source of SGR 1900+14 an interplanetary...

Bignami, after twenty years of work, managed to identify and understand Geminga, the first neutron star without radio emission, and the American Astronomical...

HD 44780 50554 63433 260655 Other 2MASS 0727+1710 CXOU J061705.3+222127 Geminga Gliese 251 HAT-P-20 HAT-P-24 HAT-P-33 LB-1 PSR J0659+1414 WD J0651+2844...