IJAA  Vol.5 No.2 , June 2015
Determination of Velocity and Radius of Supernova Remnant after 1000 yrs of Explosion
ABSTRACT
Supernova explosions are described as very violent events which transfer a significant amount of energy to interstellar media and are responsible for a large variety of physical processes. This study does not discuss the actual explosion mechanisms but follows the behavior of the dynamical evolution of some selected type I and type II supernova remnant and particularly after a thousand years from their explosion and shows how the density of the medium affects the evolution and the lifetime of each remnant. By studying such behaviors, a simplified model has been proposed here for the velocity and radius of the remnant after thousand years of explosion that depends only on the density of the medium and age of the remnant. It has been found that all types of supernova remnants have similar behaviors after a thousand years from their explosion despite their origin formation. Moreover, it is demonstrated that, when those selected remnants have entered or will enter into their radiative phase, an idea on their physical properties will be obtained.

Cite this paper
Chiad, B. , Ali, L. and Hassani, A. (2015) Determination of Velocity and Radius of Supernova Remnant after 1000 yrs of Explosion. International Journal of Astronomy and Astrophysics, 5, 125-132. doi: 10.4236/ijaa.2015.52016.
References
[1]   Katunari′c, J. (2009) Massive Stars: Life and Death. Dissertation, The Ohio State University, Columbus.

[2]   Evans, J. (1998) Death of Stars. Vol. 103, Physics & Astronomy Department, George Mason University, Fairfax.

[3]   Arny, T. (1998) Exploration: An Introduction to Astronomy. 2nd Edition, McGraw-Hill Companies, New York, 390- 391.

[4]   NASA’S HEASARC: Education and Public Information (2011) Introduction to Supernova Remnants.

[5]   Roger, R. and Landecker, T. (1988) Supernova Remnants and the Interstellar Medium. Cambridge University Press, Cambridge, 12-20.

[6]   Lee, J-J., Koo, B-C., Snell, R., et al. (2012) Identification of Ambient Molecular Cloud Associated with Galactic Supernova Remnant IC443.

[7]   Theiling, M. (2009) Observation of Very High Energy Gamma Ray Emission from Supernova Remnants with VERITAS. Ph.D. Thesis, Clemson University, Clemson.

[8]   Andrew, W. (2006) Filamentary Hα; Structure in the Milky Way. Ph.D. Thesis, University of Wollongong, Wollongong.

[9]   Hnatyk, B., Petruk, O. and Telezhyns’kyi, I. (2007) Transition of Supernova Remnant from the Adiabatic Stage of Evolution to Radiative Stage. Analytical Description. Kinematics and Physics of Celestial Bodies, 23, 137-146

[10]   Candel, I. (2012) Search for Gamma-Ray Emission from Supernova Remnants with the Fermi/LAT and MAGIC Telescopes. Ph.D. Thesis, University of Aut`onoma, Barcelona.

[11]   Cioffi, D., McKee, C. and Bertschinger, E. (1988) Dynamics of Radiative Supernova Remnants. Astrophysical Journal, 334, 252-265. http://dx.doi.org/10.1086/166834

[12]   Shu, F. (1992) The Physics of Astrophysics Volume II: Gas Dynamics. University Science Books, Mill Valley.

[13]   Ali, L. (2011) Theoretical Study of the Physical Parameters of the Supernova 1987A. Master’s Thesis, University of Baghdad, Baghdad.

[14]   Ksenofontov, L.T., Voelk, H.J. and Berezhko, E.G. (2010) Non Thermal Properties of Supernova Remnant G1.9+0.3. http://arxiv.org/abs/1004.2555

[15]   Patnaude, D.J., Badenes, C., Park, S. and Laming, J.M. (2012) The Origin of Kepler’s Supernova Remnant. http://arxiv.org/abs/1206.6799

[16]   Tang, Z.M. (1986) The Dynamic Evolution of the Kepler Supernova Remnant. Astrophysics and Space, 124, 315-327. http://dx.doi.org/10.1007/BF00656043

[17]   Blair, W.P., Long, K.S. and Vancura, O. (1991) A Detailed Optical Study of Kepler’s Supernova Remnant. Astrophysical Journal, 366, 484-494. http://dx.doi.org/10.1086/169583

[18]   Hughes, J.P. (2000) The Expansion of the X-Ray Remnant of Tycho's Supernova (SN 1572). The Astrophysical Journal, 545, L53-L56. http://dx.doi.org/10.1086/317337

[19]   Winkler, P.F., Gupta, G. and Long, K.S. (2003) The SN 1006 Remnant: Optical Proper Motions, Deep Imaging, Distance, and Brightness at Maximum. The Astrophysical Journal, 585, 324-335.
http://dx.doi.org/10.1086/345985

[20]   Chiad, B.T., Karim, L.M. and Ali, L.T. (2012) Study the Radial Expansion of SN 1987A Using Counting Pixels Method. International Journal of Astronomy and Astrophysics, 2, 199-203.
http://dx.doi.org/10.4236/ijaa.2012.24025

[21]   Dwarkadas, V.V. (2006) Supernova Explosions in Winds and Bubbles with Applications to SN 1987A.
http://arxiv.org/abs/astro-ph/0612665

[22]   Hwang, U. and Laming, J.M. (2011) A Chandra X-Ray Survey of Ejecta in the Cassiopeia A Supernova Remnant. http://arxiv.org/abs/1111.7316

[23]   Henry, R.C., Fritz, G., Meekins, J.F., Chubb, T.A. and Friedman, H. (1972) Absorption of Crab Nebula X-Ray. Astrophysical Journal, 174, 389-397. http://dx.doi.org/10.1086/151498

[24]   http://en.wikipedia.org/wiki/Crab_Nebula

[25]   Bietenholz, M.F., Kronberg, P.P., Hogg, D.E. and Wilson, A.S. (1991) The Expansion of the Crab Nebula. Astrophysical Journal, 373, L59-L62. http://dx.doi.org/10.1086/186051

[26]   Blair, W.P., Sankrit, R., Raymond, J.C. and Long, K.S. (1999) Distance to the Cygnus Loop from Hubble Space Telescope Imaging of the Primary Shock Front. The Astronomical Journal, 118, 942-947. http://dx.doi.org/10.1086/300994

[27]   Martinez, A.P. (2010) The Cygnus Loop: A Weak Core-Collapse SN in Our Galaxy. Astronomy & Astrophysics, 527, A55. http://dx.doi.org/10.1051/0004-6361/201015213

[28]   Nemes, N. (2005) XMM-Newton Observation of the Northeastern Limb of the Cygnus Loop Supernova Remnant. Ph.D. Thesis, Osaka University, Osaka.

[29]   Kirshner, R.P. and Taylor, K. (1976) High-Velocity Gas in the Cygnus Loop. The Astronomical Journal, 208, L83-L86. http://dx.doi.org/10.1086/182237

[30]   Rho, J., Jarrett, T.H., Cutri, R.M. and Reach, W.T. (2001) Near-Infrared Imaging and [O~I] Spectroscopy of IC 443 Using 2MASS and ISO. The Astrophysical Journal, 547, 885-898.
http://dx.doi.org/10.1086/318398 http://arxiv.org/abs/astro-ph/0010551

[31]   Hnatyk, B. and Petruk, O. (1998) Supernova Remnants as Cosmic Ray Accelerators. SNR IC 443. Condensed Matter Physics, 1, 655-667. http://dx.doi.org/10.5488/CMP.1.3.655

[32]   Zhang, Z.Y., Gao, Y. and Wang, J.Z. (2010) CO Observation of SNR IC 443. Science China: Physics, Mechanics & Astronomy, 53, 1357-1369.

[33]   Lee, J.J., Koo, B.C., Yun, M.S., Stanimirovic, S., Heiles, C. and Heyer, M. (2008) A 21 cm Spectral and Continuum Study of IC443 Using the Very Large Array and the ARECIBO Telescope. The Astronomical Journal, 135, 796-808. http://dx.doi.org/10.1088/0004-6256/135/3/796

[34]   Truelove, J.K. and Mckee, C.F. (1999) Evolution of Nonradiative Supernova Remnants. The Astrophysical Journal Supplement Series, 120, 299-326. http://dx.doi.org/10.1086/313176

 
 
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