RADIOACTIVE SCANDIUM IN THE YOUNGEST GALACTIC SUPERNOVA REMNANT G1.9+0.3
Authors:
- Kazimierz J. BorkowskiKBKazimierz J. Borkowski
- Stephen P. ReynoldsSRStephen P. Reynolds
- David A. GreenDGDavid A. Green
- Una HwangUHUna Hwang
- Robert PetreRPRobert Petre
- Kalyani KrishnamurthyKKKalyani Krishnamurthy
- Rebecca WillettRWRebecca Willett
- 8 November 2010
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 724 (2) , L161-L165
Abstract
No abstract availableAll Related Versions
This publication has 27 references indexed in Scilit:
- Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?Astronomy & Astrophysics, 2010
- Search for Sc-K Line Emission from RX J0852.0$-$4622 Supernova Remnant with SuzakuPublications of the Astronomical Society of Japan, 2009
- The radio expansion and brightening of the very young supernova remnant G1.9+0.3Monthly Notices of the Royal Astronomical Society: Letters, 2008
- Improved measurement of thehalf-life from a 14-year long studyPhysical Review C, 2006
- ChandraObservations of Galactic Supernova Remnant Vela Jr.: A New Sample of Thin Filaments Emitting Synchrotron X‐RaysThe Astrophysical Journal, 2005
- XMM-Newtonobservations of the supernova remnant RX J0852.0-4622/GRO J0852-4642Astronomy & Astrophysics, 2004
- Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning‐Front PropagationThe Astrophysical Journal Supplement Series, 1999
- Gamma‐Ray Line Emission from Radioactive Isotopes in Stars and GalaxiesPublications of the Astronomical Society of the Pacific, 1998
- Standard Solar CompositionSpace Science Reviews, 1998
- Interaction of Type Ia Supernovae with Their SurroundingsThe Astrophysical Journal, 1998