Details on Acronym: [SPB2020] | |
[SPB2020] | (Sano+Plucinsky+Bamba+, 2020) |
Write: | <<[SPB2020] Cloud A>> |
N: | 9 |
Object: | MCld (SIMBAD class: MolCld = Molecular Cloud) |
Stat: | is completely incorporated in Simbad |
Note: | ALMA Band 3 observations of N=9 molecular clouds within LHA 120-N 132D. Use of archival Chandra and HST (WFPC2 and ACS) data. |
in source: | Magellanic Clouds:LMC:LHA 120-N 132D = LHA 120-N 132D |
Ref: | =2020ApJ...902...53S |
by | SANO H. , PLUCINSKY P.P., BAMBA A., SHARDA P., FILIPOVIC M.D., LAW C.J., ALSABERI R.Z.E., YAMANE Y., TOKUDA K., ACERO F., SASAKI M., VINK J., INOUE T., INUTSUKA S., SHIMODA J., TSUGE K., FUJII K., VOISIN F., MAXTED N., ROWELL G., ONISHI T., KAWAMURA A., MIZUNO N., YAMAMOTO H., TACHIHARA K., FUKUI Y. |
Astrophys. J., 902, 53-53 (2020) | |
ALMA CO observations of γ-ray supernova remnant N132D in the Large Magellanic Cloud: possible evidence for shocked molecular clouds illuminated by cosmic-ray protons. | |
o | Fig. 5, Table 2: <[SPB2020] Cloud A> (Nos A-I). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |