Details on Acronym: [VVM2018] | |
| [VVM2018] | (Veena+Vig+Mookerje+, 2018)= ([VVM2018a]) |
| Write: | <<[VVM2018] CNN>> <<[VVM2018] NIRNN>> <<[VVM2018] MIRNN>> |
| N: | 10+34+22 |
| Object: | Clump + Poss. YSO + YSO (SIMBAD class: Unknown = Object of Unknown Nature) |
| Stat. | in SIMBAD: Table 2 completely incorporated. |
| Note: | N=10 molecular clumps from Spitzer GLIMPSE and MIPSGAL, Herschel Hi-Gal, APEX+Planck data. N=34 NIR and N=22 MIR YSO candidates from 2MASS and Spitzer. |
| in source: | SDC G333.739+0.352 |
| Ref: | =2018ApJ...852...93V |
| by | VEENA V.S. , VIG S., MOOKERJEA B., SANCHEZ-MONGE A., TEJ A., ISHWARA-CHANDRA C.H. |
| Astrophys. J., 852, 93-93 (2018) | |
| Probing the massive star-forming environment: a multiwavelength investigation of the filamentary IRDC G333.73+0.37. | |
| o | Source S1 is [SPK2012] MWP1G333726+003642. Source S2 is [BBC2006] IRAS 16164-4929 Clump 2. Sources P1 and P2 are not in SIMBAD. Sources in Table 5 are all from 2MASS (acronym 2MASS JHHMMSSss+DDMMSSs), while those in Table 6 are all from GLIMPSE (acronyms SSTGLMC or SSTGLMA GLLL.llll+BB.bbbb); the nick names given by the authors as "NIRNN" and "MIRNN" will thus not be added in Simbad. |
| o | Fig. 4, Table 2: <[VVM2018] CNN> (Nos C1-C10). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [VVM2018a] | |
| [VVM2018a] | (Veena+Vig+Mookerje+, 2018) |
| ***** | Avoid the usage of [VVM2018a], prefer [VVM2018] |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |