Details on Acronym: G98 | |
G98 | (Gordon+, 1998) |
***** | Avoid the usage of G98, prefer M33SNR |
Origin | of the Acronym: L (2005AJ....130..539G) |
Details on Acronym: GKL | |
GKL | (Gordon+Kirshner+Long+) |
***** | Avoid the usage of GKL, prefer M33SNR |
Origin | of the Acronym: L (2001A&A...373..438H) |
Details on Acronym: GKL98 | |
GKL98 | (Gordon+Kirshner+Long+, 1998) |
***** | Avoid the usage of GKL98, prefer M33SNR |
Origin | of the Acronym: L (2001A&A...373..438H) |
Details on Acronym: M33:SNR | |
M33:SNR | (M 33, SNR) |
***** | Avoid the usage of M33:SNR, prefer M33SNR |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: M33SNR | |
M33SNR | (M 33, SNR)= (G98) = (GKL) = (GKL98) = (M33:SNR) |
Write: | <<M33SNR NN>> |
N: | 98 |
Object: | SNR (SIMBAD class: SNRemnant = SuperNova Remnant) |
Stat: | is completely incorporated in Simbad |
Note: | Results of search for optical supernova remnants in the galaxy M33. It is part of a larger survey to search for SNRs in optical, X-ray and radio wavelengths. The SNRs in this sample were discovered based upon their high [S II]:H-alpha ratios, and many were confirmed with followup optical spectroscopy. New supernovae designations are officially assigned only by the Central Bureau for Astronomical Telegrams (http://cfa-www.harvard.edu/iau/cbat.html) |
in source: | M 33 = NGC 598 |
Ref: | =1998ApJS..117...89G |
by | GORDON S.M. , KIRSHNER R.P., LONG K.S., BLAIR W.P., DURIC N., SMITH R.C. |
Astrophys. J., Suppl. Ser., 117, 89-None (1998) | |
A new optical sample of supernova remnants in M33. | |
o | Table 3: <M33SNR NN> (Nos 1-98) |
Origin | of the Acronym: A = Assigned by the author(s) |