Andrea Mia Ghez (1965-yil 16-iyunda tug'ilgan) - amerikalik astronom va Kaliforniya universitetining fizika va astronomiya bo'limi professori, Los-Anjeles.
Uning tadqiqotlari Somon yo'li galaktikasining markaziga qaratilgan. 2020-yilda u fizika boʻyicha Nobel mukofotining yarmini Reynxard Genzel bilan baham koʻrdi (ikkinchi yarmi Rojer Penrozga berildi) fizika boʻyicha Nobel mukofotini olgan toʻrtinchi ayol boʻldi. Nobel mukofoti Ghez va Genzelga Somon yo'li galaktika markazidagi qora tuynuk hisoblangan ixcham o'ta massali ob'ektni kashf etgani uchun berildi.
Ghez (1997). „High Spatial Resolution Imaging of Pre-Main Sequence Binary Stars: Resolving the Relationship Between Disks and Close Companions“. Astrophysical Journal. 490-jild, № 1. 353–367-bet. doi:10.1086/304856.{{cite magazine}}: CS1 maint: uses authors parameter ()
Ghez (1998). „High Proper Motions in the Vicinity of Sgr A*: Evidence for a Massive Central Black Hole“. Astrophysical Journal. 509-jild, № 2. 678–686-bet. doi:10.1086/306528.{{cite magazine}}: CS1 maint: uses authors parameter ()
Ghez (2000). „The Accelerations of Stars Orbiting the Milky Way's Central Black Hole“. Nature. 407-jild, № 6802. 349–351-bet. doi:10.1038/35030032. PMID 11014184.{{cite magazine}}: CS1 maint: uses authors parameter ()
Ghez (1 Ocak 2003). „The First Measurement of Spectral Lines in a Short-Period Star Bound to the Galaxy's Central Black Hole: A Paradox of Youth“. Astrophysical Journal Letters (İngilizce). 586-jild, № 2. L127-bet. doi:10.1086/374804. CS1 maint: unrecognized language () CS1 maint: uses authors parameter ()
Ghez (1 Ocak 2008). „Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits“. Astrophysical Journal (İngilizce). 689-jild, № 2. 1044–1062-bet. doi:10.1086/592738. CS1 maint: unrecognized language () CS1 maint: uses authors parameter ()
Fizika bo'yicha Nobel mukofoti sovrindorlari ro'yxati
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