N
Nino Panagia
Researcher at Space Telescope Science Institute
Publications - 483
Citations - 52007
Nino Panagia is an academic researcher from Space Telescope Science Institute. The author has contributed to research in topics: Supernova & Galaxy. The author has an hindex of 89, co-authored 478 publications receiving 48961 citations. Previous affiliations of Nino Panagia include Cornell University & University of Catania.
Papers
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Book ChapterDOI
IUE Observations of Supernovae
Nino Panagia,Roberto Gilmozzi +1 more
TL;DR: The launch of the International Ultraviolet Explorer (IUE) satellite in early 1978 marked the beginning of a new era for SN studies because of its capability of measuring the ultraviolet emission of objects as faint as m B = 15 as mentioned in this paper, and just around that time other powerful astronomical instruments have become available, such as the Einstein Observatory for X-ray measurements, the VLA for observations at radio wavelengths and a number of new telescopes either dedicated to infrared observations (eg UKIRT and IRTF at Mauna Kea) or equipped with new and highly efficient IR instrumentation (eg
Journal ArticleDOI
On the Pulsation Properties of Red Supergiant Variables
Giuseppe Bono,Nino Panagia +1 more
Book ChapterDOI
The Rate and the Origin of Type Ia SNe in Radio Galaxies
M. Della Valle,Nino Panagia,Nino Panagia,Enrico Cappellaro,Paolo Padovani,Paolo Padovani,Massimo Turatto +6 more
TL;DR: In this article, an analysis of type Ia supernova (SNe) events in early type galaxies from the Cappellaro et al. database provides strong evidence that the rate of SNe in radio-loud galaxies is about 4 times higher than the rate measured in radio quiet galaxies.
Journal ArticleDOI
Radio Insight into the Nature of Type IIb Progenitors
Chris Stockdale,Stuart D. Ryder,Assaf Horesh,K. W. Weiler,Nino Panagia,S. D. Van Dyk,Franz E. Bauer,Stefan Immler,Richard A. Sramek,David Pooley,J. M. Marcaide,N. E. Kassim +11 more
TL;DR: In this paper, the results of over two decades of radio observations of type IIb supernovae with the Very Large Array and the Australia Telescope Compact Array are presented, which illustrate the need for multi-wavelength follow-up to determine the progenitor scenario for type Ib events.
ON THE MULTIPLICITY OFh CARINAE
TL;DR: The luminous blue variable (LBV) h Car is extremely N rich and C and O poor, which is indicative of CNO-cycle products as mentioned in this paper. But it is not the star that ejected the nebula.