Dictionary of Nomenclature of Celestial Objects
(Last update: 18-Dec-2020)

Result of query: info cati NMV2001] Knot A$



Details on Acronym:   [NMV2001]
   [NMV2001] (Nisini+Massi+Vitali+, 2001) Write:<<[NMV2001] Knot A>>
<<[NMV2001] Outflow R>>
<<[NMV2001] YSO NN>> N: 21+3+20 Object:?  (SIMBAD class: Unknown = Object of unknown nature) Stat:is completely incorporated in Simbad Note:Jets in IC 1396N: N=21 knots, 3 outflows, and N=20 (Near-IR) YSO embedded young objects.
See also [CBN2001]. in source:IC 1396N Ref:=2001A&A...376..553N byNISINI B. , MASSI F., VITALI F., GIANNINI T., LORENZETTI D., DI PAOLA A., CODELLA C., D'ALESSIO F., SPEZIALI R. Astron. Astrophys., 376, 553-560 (2001) Multiple H_2 protostellar jets in the bright-rimmed globule IC 1396-N. oInversion of position between table 1 and fig 4 : D and F objects. oTable 1, Fig.4: <[NMV2001] Knot A> (Nos A-G). Fig.5: <[NMV2001] Outflow R> (Nos I to III). Table 2: <[NMV2001] YSO NN> (Nos 1-20). Ref:=2003ApJ...593L..47R byREIPURTH B. , ARMOND T., RAGA A., BALLY J. Astrophys. J., 593, 47-50 (2003) Blowout from IC 1396N: the emergence of Herbig-Haro flows from a cloud core. oFig.3: <[NMV2001] Knot A> (Nos H-M) added. Ref:=2006A&A...449.1077C byCARATTI O GARATTI A. , GIANNINI T., NISINI B., LORENZETTI D. Astron. Astrophys., 449, 1077-1088 (2006) H_{2} active jets in the near IR as a probe of protostellar evolution. oFig.11, Table 7: <[DE95] NGC 2264G AN> (Nos I1-I5, H1-H5) added. Fig.12, Table 7: <[CGN2006] VLA 1623 A> (Nos A-D). Fig.12, Table 7: <[GSWC2003] NNa> (Nos 14h, 14i, 17b) added. Fig.17, Table 7: <[NMV2001] Knot A> (Nos N-R) added. Ref:=2009A&A...504...97B byBELTRAN M.T. , MASSI F., LOPEZ R., GIRART J.M., ESTALELLA R. Astron. Astrophys., 504, 97-107 (2009) The stellar population and complex structure of the bright-rimmed cloud IC 1396N. oTables 1-4: <[BML2009] NIR NNNNA> N=736. Table 5: <[NMV2001] Knot A> (Nos T-V) added, <[BML2009] ANN> N=88. =E=Catalogue in electronic form as J/A+A/504/97 Originof the Acronym: S = Created by Simbad, the CDS Database

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