V4998 Sagittarii
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Sagittarius IAU.svg
Författare/Upphovsman: IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg), Licens: CC BY 3.0
IAU Sagittarius chart
Författare/Upphovsman: IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg), Licens: CC BY 3.0
IAU Sagittarius chart
V4998SgrLightCurve.png
Författare/Upphovsman: PopePompus, Licens: CC BY-SA 4.0
A near-infrared (K band) light curve for V4998 Sagittarii, adapted from Mauerhan et al., The Astrophysical Journal Letters, 713:L33–L36, 2010 April 10
Författare/Upphovsman: PopePompus, Licens: CC BY-SA 4.0
A near-infrared (K band) light curve for V4998 Sagittarii, adapted from Mauerhan et al., The Astrophysical Journal Letters, 713:L33–L36, 2010 April 10
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Quintuplet cluster region (1002.3379).jpg
Hubble Space Telescope image of the Quintuplet Cluster region. The Pistol Star is seen in the middle, surrounded by its ejection nebula. The luminous blue variable (LBV) star G0.120−0.048 is at the upper right, surrounded by a spherical nebula, believed to have been ejected by that star. LBV qF362 to the left of the Pistol Star also seems to be surrounded by a low-level nebular emission.
Hubble Space Telescope image of the Quintuplet Cluster region. The Pistol Star is seen in the middle, surrounded by its ejection nebula. The luminous blue variable (LBV) star G0.120−0.048 is at the upper right, surrounded by a spherical nebula, believed to have been ejected by that star. LBV qF362 to the left of the Pistol Star also seems to be surrounded by a low-level nebular emission.
LBV G0.120-0.048.jpg
Hubble Space Telescope image of the luminous blue variable (LBV) star G0.120−0.048, surrounded by a spherical nebula believed to have been ejected by that star.
Hubble Space Telescope image of the luminous blue variable (LBV) star G0.120−0.048, surrounded by a spherical nebula believed to have been ejected by that star.