Multi-wavelength Atlas of Molecular Supernova Remnants
This is page is supported by Long-Term Space Astrophysics program. When
you use this archival products, please cite the references given for each
image and this page.
This page is maintained by Dr. Jeonghee Rho who is the PI of LTSA proposal
of "A multi-wavelength study of Molecular Supernova remnants".
| Evidence of interaction | X-ray image | radio image | Near-IR images | Mid- and Far- Infrared
images |
|
| W44(G34.7-0.4) | Broad CO line
Infrared cooling line of [OI] |
X-ray ROSAT PSPC image
in fits
(Rho et al. 1994, ApJ, 430, 757) |
W44 radio image in fits
(Jones et al. 1993, MNRAS,265, 631) |
NA (not availlable yet) |
NA |
| W28(G6.4-0.1) | Broad CO line
Infrared cooling line of [OI] |
X-ray ROSAT PSPC images
in fits
(Rho & Borkowski, 2002, ApJ, 581, 1112) |
Radio image of W28
(Frail et al. 1999) |
NA | NA |
| 3C391(G31.9+0.0) | Broad CO line
Infrared cooling line of [OI] |
.X-ray ROSAT PSPC image in fits
(Rho & Petre, 1996, ApJ, 467, 698) |
NA | NA | NA |
| IC443 | Broad CO line
Infrared cooling line of [OI] |
NA | NA | NA | NA |