Accretion_Disk_Binary_System.jpg (800 × 525 pixels, file size: 24 KB, MIME type: image/jpeg)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 23:58, 24 January 2008 | 800 × 525 (24 KB) | Ilmari Karonen | *{{en|Accretion Disk Binary System. NASA's explanation: :Our Sun is unusual in that it is alone - most stars occur in multiple or binary systems. In a binary system, the higher mass star will evolve faster and will eventually become a compact object - eit |
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More than 100 pages use this file. The following list shows the first 100 pages that use this file only. A full list is available.
- 14 Aquarii
- 4U 0142+61
- AXP 1E 1048-59
- Accretion (astrophysics)
- Alpha2 Canum Venaticorum variable
- Anomalous X-ray pulsar
- BG Geminorum
- Binary star
- DI Lacertae
- DM Geminorum
- DM Lyrae
- EO Aurigae
- FO Aquarii
- G 185-32
- Gliese 22
- HAT-P-5
- HD 118508
- HD 123657
- HD 126141
- HD 126200
- HD 126271
- HD 127726
- HD 128333
- HD 130948
- HD 135530
- HD 151967
- HD 153201
- HD 155035
- HD 158220
- HD 182475
- HD 194244
- HD 202259
- HD 211392
- HD 219659
- HD 220035
- HD 221148
- HD 223229
- HR Lyrae
- IZ Aquarii
- Irregular variable
- LHS 292
- LP Aquarii
- OGLE-TR-113
- OGLE-TR-132
- OGLE-TR-56
- PSR B0329+54
- PSR B0950+08
- PSR B1259−63/LS 2883
- PSR B1828−11
- PSR B1829−10
- PSR J0537−6910
- PSR J0855−4644
- PSR J1903+0327
- PSR J1951+1123
- PSR J2144−3933
- PU Aurigae
- QS Aquilae
- R Canum Venaticorum
- R Corvi
- R Horologii
- R Reticuli
- R Virginis
- Rotating ellipsoidal variable
- SAX J1808.4−3658
- SN 1986G
- SN 1990U
- SN 1992bd
- SN 1994D
- SN 1998S
- SN 1999ec
- SN 1999eu
- SN 2003B
- SN 2003H
- SN 2004dj
- SN 2004gt
- SN 2005B
- SN 2005bc
- SN 2006X
- SN 2007sr
- SWIFT J1756.9−2508
- S Virginis
- T Andromedae
- Type Ia supernova
- UX Tauri
- V1059 Sagittarii
- V1339 Aquilae
- V385 Andromedae
- V394 Aurigae
- V433 Aurigae
- V446 Herculis
- V450 Aquilae
- V604 Aquilae
- V606 Aquilae
- V744 Centauri
- V849 Ophiuchi
- WASP-10
- WASP-14
- WASP-4
- W Virginis variable
- Z Apodis
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