M
Massimo Marengo
Researcher at Iowa State University
Publications - 233
Citations - 14103
Massimo Marengo is an academic researcher from Iowa State University. The author has contributed to research in topics: Stars & Spitzer Space Telescope. The author has an hindex of 52, co-authored 228 publications receiving 13242 citations. Previous affiliations of Massimo Marengo include University of Arizona & International School for Advanced Studies.
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New Evidence for Mass Loss from δ Cephei from H I 21 cm Line Observations
TL;DR: In this article, the authors used the H I 21 cm line observations with the Very Large Array (VLA) to search for neutral atomic hydrogen associated with a stellar wind, showing that a mass loss of this magnitude, sustained over the preceding Cepheid lifetime of the star, could be sufficient to resolve a significant fraction of the discrepancy between the pulsation and evolutionary masses for this star.
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Infrared observations of the helix planetary nebula
TL;DR: In this article, the authors have mapped the Helix (NGC 7293) planetary nebula (PN) with the IRAC instrument on the Spitzer Space Telescope, which resolved the "cometary knots" and the radial rays extending into the outer regions of the PN.
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On the distance of the globular cluster m4 (ngc 6121) using rr lyrae stars. ii. mid-infrared period–luminosity relations
Jillian R. Neeley,Massimo Marengo,Giuseppe Bono,V. F. Braga,Massimo Dall'Ora,Peter B. Stetson,R. Buonanno,I. Ferraro,Wendy L. Freedman,G. Iannicola,Barry F. Madore,Noriyuki Matsunaga,A. Monson,S. E. Persson,Victoria Scowcroft,Mark Seibert +15 more
TL;DR: In this article, the authors presented mid-infrared period-luminosity (PL) relations for RR Lyrae variables in the globular cluster M4 (NGC 6121) using observations from the Infrared Array Camera onboard the Spitzer Space Telescope.
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A wide-field near- and mid-infrared census of young stars in ngc 6334
TL;DR: In this article, the authors presented a study of the rate and efficiency of star formation in the NGC 6334 star-forming region using the NOAO Extremely Wide-Field Infrared Imager and combined them with observations taken with the Infrared Array Camera (IRAC) on the Spitzer Space Telescope at wavelengths = 3.6, 4.5, 5.8, and 8.0 μm.
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Spitzer observations of NGC 2264: the nature of the disk population
TL;DR: In this article, the authors studied the star formation history of NGC2264 and analyzed the primordial disk evolution of its members using data obtained with the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer for Spitzer (MIPS) on board the Spitzer Space Telescope, combined with deep near-infrared (NIR) ground-based FLAMINGOS imaging and previously published optical data.