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Nova remnant
Exploring Pulsars
Reconsidering the Identification of M101 Hypernova Remnant
Wind-Blown Bubbles and Hii Regions Around Massive
Ghost Supernova Remnants: Evidence for Pulsar Reactivation in Dusty Molecular Clouds?
Blasts from the Past Historic Supernovas
Supernova Remnant N103B, Radio Pulsar B1951+32, and the Rabbit
Observing Bright Nebulae
Astronomy General Information
IAUS283 Planetary Nebulae: an Eye to the Future P R O G R a M M E & a B S T R a C
The Evolution of Nova Remnants
Te11 As the Remnant of Nova Ori AD 483
Redalyc.SUPERNOVA REMNANTS: a LINK BETWEEN MASSIVE STARS
Old and New Neutron Stars*
Supernova Remnants: the X-Ray Perspective
Kristiina Verro Physical Properties of the Nova Remnant Nova Persei 1901
Neutrinos from the Pulsar Wind Nebulae
Study the Radial Expansion of SN 1987A Using Counting Pixels Method
Star Formation and Molecular Clouds Towards the Galactic Anti-Center
Top View
Supernova Remnant Shocks in an Inhomogeneous Interstellar Medium
Discovery of an Old Nova Remnant in the Galactic Globular Cluster M 22? Fabian Göttgens1, Peter M
The Supernova
Evolution of Red Nova V4332 Sagittarii Remnant E
Modelling the Structure and Kinematics of the Firework Nebula: the Nature
Astronomers' Universe ISBN 978-3-030-10379-8 ISBN 978-3-030-10380-4 (Ebook)
Non-Thermal Radio Supernova Remnants of Exiled Wolf-Rayet Stars
Black Holes, Pulsars, and More
Supernova Remnant SN 1006
Supernova Educator Guide (PDF)
A 300 Parsec Long Jet-Inflated Bubble Around a Powerful Microquasar in the Galaxy NGC 7793
Nova Gk Persei - a Miniature Supernova Remnant?
Arxiv:1406.4364V1 [Astro-Ph.HE] 17 Jun 2014 E-Mail:
[email protected]
2 Patrick Slane Et Al
Pos(ICRC2021)983
Redalyc.H 2-12, a Misidentified Planetary Nebula in Kepler
Astronomy Div C 2014 Help Session V0
A Physical Interpretation of the Jet-Like X-Ray Emission from Supernova
Download This PDF File
Discovery of an Old Nova Remnant in the Galactic Globular Cluster M 22 Fabian Göttgens1, Peter M
Progress Report and Highlights Martin C. Weisskopf the Chandra X-Ray Observatory, the Third of NA
Mutual Influence of Supernovae and Molecular Clouds⋆
Neutron Star Astronomy at ESO: the VLT Decade
Redalyc.Wind-Blown Bubbles and HII Regions Around Massive Stars
3) 'The Unusual Supernova Remnant Surrounding the Ultraluminous X-Ray Source IC 342 X-1.', Monthly Notices of the Royal Astronomical Society., 342 (3)
A Non-Pulsating Neutron Star in the Supernova Remnant HESS J1731−347/G353.6−0.7 with a Carbon Atmosphere
Curriculum Vitae ROBERT A. FESEN Address
Study of Molecular Clouds in the Vicinity of Supernova Remnants As Sources of Very-High-Energy Gamma-Ray Emission
A Critical Examination of Hypernova Remnant Candidates in M101. II. NGC 5471B C-HR Chen
The Vela Supernova Remnant and Surrounds – a Photographic Tour
A Multiwavelength Study of the Remnant of Nova GK Persei
In the Chandra Era
Pulsar Wind Nebulae: Theoretical Aspects and Observational Constraints
The Physics of Asymmetric Supernovae and Supernovae Remnants
Optical Imaging and Spectroscopy of the Galactic Supernova Remnant 3C 58 (G130.7+3.1) Robert Fesen Dartmouth College