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X-ray pulsar in the constellation Gemini
Geminga (/ɡəˈmɪŋɡə/ gə-MING-gə) is a gamma ray and x-ray pulsar source thought to be a neutron star approximately 250 parsecs (around 800 light-years)
Geminga
Zodiac constellation in the northern hemisphere
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
Gemini_(constellation)
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
List_of_proper_names_of_stars
Milky Way superbubble
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
Local_Bubble
Italian astrophysicist (born 1954)
first unidentified pulsar radio emission, she identified the neutron star Geminga. She has developed a multi-wavelength strategy for the identification of
Patrizia_Caraveo
Star in the constellation Orion
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
Meissa
Supernova remnant in the constellation Vela
of the closest known to Earth, being around 800 light years away. The Geminga pulsar is closer (and also resulted from a supernova), and in 1998 another
Vela_supernova_remnant
Planets found orbiting pulsars
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
Pulsar_planet
Supernova close enough to affect Earth's biosphere
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
Near-Earth_supernova
Particle detector on the International Space Station
pulsar Geminga. The accelerated electrons and positrons collide with nearby starlight. The collision boosts the light to much higher energies. Geminga alone
Alpha_Magnetic_Spectrometer
Isolated radio pulsar in the constellation Camelopardalis
small angle between the spin axis and line of sight, similar to the pulsar Geminga. No termination shock is evident, and comparisons with other PWNs like
PSR_B0355+54
Italian physicist (1944–2017)
Italian astrophysicist, best known for his discovery of the neutron star Geminga. From March 2007 until August 2008, he was Chairman of the Italian Space
Giovanni_Bignami
American astrophysicist
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
Neil_Gehrels
Cosmic ray research module
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
PAMELA_detector
Gamma ray telescope
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
Small_Astronomy_Satellite_2
Neutron star that does not emit radio waves
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
Radio-quiet_neutron_star
Planetary nebula in constellation Gemini
nebula is a PG 1159 star. Abell Catalog of Planetary Nebulae Geminga, Gemini gamma-ray source Gemini in Chinese astronomy IC 444, reflection
Medusa_Nebula
Satellite X-ray telescope
diffuse X-ray emission by molecular clouds. Detection of pulsations from Geminga. Detection of isolated neutron stars. Discovery of X-ray emission from
ROSAT
Observational astronomy performed with gamma rays
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
Gamma-ray_astronomy
Binary star system in the constellation Gemini
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
Sigma_Geminorum
Star in the constellation Gemini
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
Theta_Geminorum
G-type star in the constellation Gemini
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
Iota_Geminorum
Binary star system in the constellation Gemini
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
Kappa_Geminorum
Astronomical object
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
Optical_pulsar
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
Indirect detection of dark matter
Indirect_detection_of_dark_matter
the measurements of the pulsed optical emission from PSR B0656+14 and Geminga (Src). JPL · 11450 11451 Aarongolden 1979 QR1 Aaron Golden (born 1969)
Meanings of minor-planet names: 11001–12000
Meanings_of_minor-planet_names:_11001–12000
Star in the constellation Gemini
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
Omicron_Geminorum
Binary star system in the constellation Gemini
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
Phi_Geminorum
Evolved red giant star in the constellation Gemini
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
Upsilon_Geminorum
Star system in the constellation Gemini
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
Nu_Geminorum
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
List_of_stars_in_Gemini
Observatory
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
Pushchino Radio Astronomy Observatory
Pushchino_Radio_Astronomy_Observatory
Turkish astrophysicist (1940–2011)
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
Hakkı_Ögelman
Star in the constellation Gemini
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
Omega_Geminorum
Star in the constellation of Gemini
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
Chi_Geminorum
School in Milan, Italy
Bignami, after twenty years of work, managed to identify and understand Geminga, the first neutron star without radio emission, and the American Astronomical
Milan_school_of_physics
Star in the constellation Gemini
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
Pi_Geminorum
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Girl/Female
Muslim
Fairy faced
Surname or Lastname
English
English : topographic name for someone who lived at the foot of a hill, or a habitational name from Underhill in Devon, named from Old English under ‘under’ + hyll, or from Underhill in Kent, named from Old English under + helde ‘slope’.John Underhill (c.1597–1672) was born in Kenilworth, Warwickshire, England. His father was a mercenary in the Netherlands, and he himself became a cadet in the Prince of Orange’s guards. In 1630 he emigrated to Boston, MA, where he was appointed captain of militia. In 1664–65 he played a significant role in helping to bring the Dutch colony of New Netherland under English control.
Girl/Female
Assamese, Gujarati, Hindu, Indian, Sindhi
Raga in Hindustani Classical Music
Boy/Male
Hindu, Indian, Kannada, Malayalam, Marathi, Oriya, Telugu
Pure Moon
Boy/Male
Hindu
Lord of Vedas a Hindu mythologys detail knowledge
Male
Irish
Old Irish name thought to probably be derived from the word niadh, NIUL means "champion."
Boy/Male
Muslim/Islamic
Name of a Surah in the Quran
Biblical
estimation; thought
Male
English
Latin name derived from the word silvester, from silva, SILVESTER means "forest, wood," hence "from the forest."
Girl/Female
Australian, Irish
Saint Name
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