Long Slit Echelle Spectroscopy of Supernova Remnants in M33 Academic Article

abstract

• AbstractWe have obtained long slit echelle spectroscopy for 10 of the brightest supernova remnants in M33 using the KPNO 4 m telescope. The profiles at H indicate bulk motions in the range 100350 km s1 in these remnants. Nearly all of the objects show signs of contamination by low velocity H II emission at some level. This affects the line intensities measured from low resolution data and may affect diameter measurements of these remnants.

authors

• Kennicutt, Robert

published proceedings

• International Astronomical Union Colloquium

author list (cited authors)

• Blair, W. P., Chu, Y., & Kennicutt, R. C.

citation count

• 0

complete list of authors

• Blair, William P||Chu, You-Hua||Kennicutt, Robert C

publication date

• January 1988

publisher

• Cambridge University Press (CUP)  Publisher

published in

• International Astronomical Union Colloquium  Journal

Digital Object Identifier (DOI)

• 10.1017/s0252921100102350

start page

• 193

end page

• 196

volume

• 101

URL

• http://dx.doi.org/10.1017/s0252921100102350