Fig. 1 from Galactic Bulges from Hubble Space Telescope Near‐Infrared Camera Multi‐Object Spectrometer Observations: The Lack of r1/4 Bulges

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Galactic Bulges from Hubble Space Telescope Near‐Infrared Camera Multi‐Object Spectrometer Observations: The Lack of r^1/4 Bulges

Authors: Marc Balcells, Alister W. Graham, Lilian Domínguez-Palmero, and Reynier F. Peletier

Balcells et al. 2003 The Astrophysical Journal Letters 582 L79.

Provider: AAS Journals

Caption: Fig. 1.

(a) Combined HST plus ground‐based H‐band surface brightness profile of NGC 5443 (Sb), with PSF‐convolved Sérsic bulge and exponential disk components (solid lines). The residuals (data minus model) are shown in the lower panel. (b) Same surface brightness profile fitted with a PSF‐convolved Sérsic law, an exponential disk, plus a central PS (dashed line). Residuals are shown in the lower panel.

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