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3C 58
FY08 Technical Papers by GSMTPO Staff
Федеральное Государственное Бюджетное Учреждение Науки Физический Институт Им
7.5 X 11.5.Doubleline.P65
The Iso Handbook
Search for Very High-Energy Gamma-Ray Emission from Pulsar-Pwn Systems with the Magic Telescope
The Very High Energy Characteristics of Shell-Type Snrs and Pulsar Wind Nebulae at Different Ages
Supernova Remnants and the Life Cycle of Interstellar Dust
Exoplanet Secondary Atmosphere Loss and Revival Edwin S
X-Ray Properties of the Pulsar Psr J0205+6449 in 3C 58
Sommaire Des Annexes
Les Jeunes Vestiges De Supernova Et INTEGRAL:Raies Du 44Ti Et
High Energy Astrophysics Is One of the Most Important and Exciting Areas of Contemporary Astronomy, Involving the Most Energetic Phenomena in the Universe
XMM-Newton Eric Gotthelf (Columbia University)
Arxiv:1409.5746V4
Optical Imaging and Spectroscopy of the Galactic Supernova Remnant 3C 58 (G130.7+3.1)
Supernova Remnant 3C 58: Implications for When Acceleration Occurs
A Nearby Transiting Rocky Exoplanet That Is Suitable for Atmospheric Investigation
Events: General Meeting
Top View
Investigating the Pulsar Wind Nebula 3C 58 Using Emission
Meteor 35. Évf. 2. Sz. (2005. Február)
Planck Intermediate Results XXXI
Appendix I. Observing Programs 2009B and 2010A
Astrophysics of Hot Plasma in Extended X-Ray Sources
Distance and Age of the Pulsar Wind Nebula 3C 58 R
Curriculum Vitae ROBERT A. FESEN Address
Astronomy Magazine 2015 Index
ATMOSPHERE-INTERIOR EXCHANGE on HOT ROCKY EXOPLANETS Edwin S
Discovery of Tev Gamma-Ray Emission from the Pulsar Wind Nebula 3C 58 by MAGIC
Exoplanet Secondary Atmosphere Loss and Revival
February 2021 BRAS Newsletter
PDF of the Talk
Observing Iumman) Observatory 2002
Discovery of Pulsations from the Pulsar J0205+6449 in Snr 3C 58 with the Fermi Gamma-Ray Space Telescope
In the Chandra Era
X-Ray and Radio Timing of the Pulsar in 3C 58