Nino Panagia
Astronomer Nino Panagia (pronounced Pahn-ah-gee-ah)
was born and grew up in Rome, Italy. He earned
his doctorate in Physics at Rome
University in 1966, with a thesis on theoretical
models of massive stars. Soon afterwards he
turned his interest to the study of nebulae
and stellar winds.
In the late '60s and early '70s he held positions
at the Institute for Space Astrophysics in Frascati,
near Rome, and in Bologna, at the
Institute
of Radioastronomy. During this time, he broadened
his interests from studies at optical and ultraviolet
wavelengths to include also work on the radio
and infrared properties of nebulae. He spent
a year at Cornell University,
collaborating with Yervant
Terzian and others, where he started a series
of model calculations of the far-infrared emission
from nebulae.
In 1979 he assumed leadership of a European team
that carried out observations of supernovae
with the International Ultraviolet Explorer
(IUE) satellite. This was the beginning of
Panagia's long-term involvement with supernova
studies (and made him an observational astronomer,
in addition to his theoretical credentials).
His team's approach involved using observations
at many different wavelengths (spanning from radio
to gamma rays) to understand the nature of stellar
explosions.
In 1984 Nino came to the Space Telescope
Science Institute. From 1986 to 1995,
however, he also tried to be in two places at once,
since he was appointed Professor of Astronomy and
taught part-time at the University
of Catania (Sicily). Since 1995 he has worked
full time at STScI. His current Institute work is
involved with the James
Webb Space Telescope project.
His research activity on supernovae led to the
first thorough study of the radio emission from
a supernova (SN 1979C, which is still being
followed with the Very Large Array radio
telescope), and the first detailed study
of the new class of Type Ib supernovae. Since
the launch of HST, Panagia has been involved
in a detailed study of the supernova in the
Large Magellanic Cloud, SN
1987A, and its vicinity. This work led to determination
of a very precise distance to the LMC, which
is a fundamental step in the cosmological
distance-scale ladder.
When he is not doing astronomy, Nino listens to
Baroque music, spends time in the kitchen (where
he is a master of southern Italian cooking),
gardens, and takes long walks in his neighborhood.
During vacations he can be found snorkeling
in the Caribbean.
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