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How similar is the stellar structure of low-mass late-type galaxies to that of early-type dwarfs?
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X-RAY CONSTRAINTS ON THE LOCAL SUPERMASSIVE BLACK HOLE OCCUPATION FRACTION
The Herschel Virgo Cluster Survey – XIV. Transition-type dwarf galaxies in the Virgo cluster
Ilse De Looze, Maarten Baes, Alessandro Boselli, et al. Monthly Notices of the Royal Astronomical Society 436(2) 1057 (2013) https://doi.org/10.1093/mnras/stt1626
Infrared surface photometry of dwarf galaxies in Fornax
UV Properties of Early-Type Galaxies in the Virgo Cluster
A. Boselli, L. Cortese, J. M. Deharveng, et al. The Astrophysical Journal 629(1) L29 (2005) https://doi.org/10.1086/444534
POX 52: A Dwarf Seyfert 1 Galaxy with an Intermediate‐Mass Black Hole
Aaron J. Barth, Luis C. Ho, Robert E. Rutledge and Wallace L. W. Sargent The Astrophysical Journal 607(1) 90 (2004) https://doi.org/10.1086/383302
Strategies for Imaging Faint Extended Sources in the Near‐Infrared
Ovidiu Vaduvescu and Marshall L. McCall Publications of the Astronomical Society of the Pacific 116(821) 640 (2004) https://doi.org/10.1086/421854
Galaxy Populations and Evolution in Clusters. IV. Deep HiObservations of Dwarf Elliptical Galaxies in the Virgo Cluster
Christopher J. Conselice, Karen O’Neil, John S. Gallagher and Rosemary F. G. Wyse The Astrophysical Journal 591(1) 167 (2003) https://doi.org/10.1086/375216
UV to radio centimetric spectral energy distributions of optically-selected late-type galaxies in the Virgo cluster
1.65 Micron (HBand) Surface Photometry of Galaxies. X. Structural and Dynamical Properties of Elliptical Galaxies
Stefano Zibetti, Giuseppe Gavazzi, Marco Scodeggio, Paolo Franzetti and Alessandro Boselli The Astrophysical Journal 579(1) 261 (2002) https://doi.org/10.1086/342707
Spectrophotometry of Galaxies in the Virgo Cluster. I. The Star Formation History
G. Gavazzi, C. Bonfanti, G. Sanvito, A. Boselli and M. Scodeggio The Astrophysical Journal 576(1) 135 (2002) https://doi.org/10.1086/341730
1.65-μm (H-band) surface photometry of galaxies - VIII. The near-IRκspace atz=0