Details on Acronym: ISO
ISO (Infrared Source Obs.) ***** Avoid the usage of ISO, prefer ISO-Oph Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-Oph
ISO-Oph (ISO, Oph)= (ISO) Write:<<ISO-Oph NNN>>
<<ISO-Oph NNNa>> N: 212+11 Object:(IR) (SIMBAD class: Infrared = Infra-Red Source) Note:ISOCAM observations of rho Oph Cloud.
The IR stars are sometimes multiple: format NNNa. in source:NAME rho Oph Cloud Ref:=2001A&A...372..173B byBONTEMPS S. , ANDRE P., KAAS A.A., NORDH L., OLOFSSON G., HULDTGREN M., ABERGEL A., BLOMMAERT J., BOULANGER F., BURGDORF M., CESARSKY C.J., CESARSKY D., COPET E., DAVIES J., FALGARONE E., LAGACHE G., MONTMERLE T., PERAULT M., PERSI P., PRUSTI T., PUGET J.L., SIBILLE F. Astron. Astrophys., 372, 173-194 (2001) ISOCAM observations of the ρ Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster. oTable 1: <ISO-Oph NNN> (Nos 1-212). Ref:=2006A&A...452..245N byNATTA A. , TESTI L., RANDICH S. Astron. Astrophys., 452, 245-252 (2006) Accretion in the ρ-Ophiuchi pre-main sequence stars. oTables C1, C2, C3: <ISO-Oph NNNa> N=11 added. =E=Catalogue in electronic form as J/A+A/372/173 =E=Catalogue in electronic form as J/A+A/452/245 Originof the Acronym: A = Assigned by the author(s)
© Université de Strasbourg/CNRS
• Contact