Details on Acronym: S68N | |
S68N | (Sh 2-68N) |
***** | Avoid the usage of S68N, prefer [WM2000] |
Origin | of the Acronym: L (2007ApJ...669..493W) |
Details on Acronym: [WM2000] | |
[WM2000] | (Williams+Myers, 2000)= (S68N) = ([WM2000a]) |
Write: | <<[WM2000] S68Na>> <<[WM2000] QN>> |
N: | 3+8 |
Object: | Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud) |
Note: | Fig.1, Table 1: N=3 continuum sources (Nos b-d) near Sh 2-68N. Fig.2, Table 2: N=8 quiescent cores (Nos Q1-Q8). |
in source: | NAME Serpens NW Cluster |
Ref: | =2000ApJ...537..891W |
by | WILLIAMS J.P. , MYERS P.C. |
Astrophys. J., 537, 891-903 (2000) | |
Evidence for pressure-driven flows and turbulent dissipation in the Serpens NW cluster. | |
o | S68N = Sh 2-68N in SIMBAD |
o | Fig.1, Table 1: <[WM2000] S68Na> (Nos S68Na to S68Nd). Fig.2, Table 2: <[WM2000] QN> (Nos Q1-Q8). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [WM2000a] | |
[WM2000a] | (Williams+Myers, 2000) |
***** | Avoid the usage of [WM2000a], prefer [WM2000] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |