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Details on Acronym: [PWM2013]
[PWM2013] (Pillitteri+Wolk+Megeath+, 2013) Write:<<[PWM2013] NNN>> N: 12 Object:(IR) (SIMBAD class: Infrared = Infra-Red Source) Note:N=10 transitional disk objects and N=2 faint objects in L1641 and ι Ori region.
Use of XMM-Newton and Spitzer data.
See also SOXS. in source:Ori A = NAME ORION NEBULA in source:Orion Nebula:LDN 1641 = LDN 1641 Ref:=2013ApJ...768...99P byPILLITTERI I. , WOLK S.J., MEGEATH S.T., ALLEN L., BALLY J., GAGNE M., GUTERMUTH R.A., HARTMAN L., MICELA G., MYERS P., OLIVEIRA J.M., SCIORTINO S., WALTER F., REBULL L., STAUFFER J. Astrophys. J., 768, 99 (2013) An X-ray survey of the young stellar population of the Lynds 1641 and ι Orionis regions. o(Erratum) erratum vol. 773, art. 80 (2013) oTables 2-4: <SOXS NNNN> (Nos 1-1060). Table 5: <[PWM2013] NNN> N=12 among (Nos 13-468). =E=Catalogue in electronic form as J/ApJ/768/99 Originof the Acronym: S = Created by Simbad, the CDS Database
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