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Details on Acronym: [UKO2005]
[UKO2005] (Uzpen+Kobulnicky+Olsen+, 2005) Write:<<[UKO2005] NN>> N: 33 Object:(Mid IR) (SIMBAD class: Star) Stat:is completely incorporated in Simbad Note:Spitzer IRAC photometry as part of the GLIMPSE survey. See also GLIMPSE. Ref:=2005ApJ...629..512U byUZPEN B. , KOBULNICKY H.A., OLSEN K.A.G., CLEMENS D.P., LAURANCE T.L., MEADE M.R., BABLER B.L., INDEBETOUW R., WHITNEY B.A., WATSON C., WOLFIRE M.G., WOLFF M.J., BENJAMIN R.A., BANIA T.M., COHEN M., DEVINE K.E., DICKEY J.M., HEITSCH F., JACKSON J.M., MARSTON A.P., MATHIS J.S., MERCER E.P., STAUFFER J.R., STOLOVY S.R., BACKMAN D.E., CHURCHWELL E. Astrophys. J., 629, 512-525 (2005) Identification of main-sequence stars with mid-infrared excesses using GLIMPSE: β Pictoris analogs? oTables 1, 2: <[UKO2005] NN> (Nos 1-33). Originof the Acronym: L = Found in the literature
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