منابع مشابه
Radio sources at low Galactic latitudes
High-resolution radio observations of a sample of 65 radio sources at low Galactic latitudes are presented. The sources were all observed at 5 GHz with the VLA A-array. MERLIN observations at 5 GHz of the ultracompact H ii region G34.26+0.15 and one of the extragalactic sources, B1857−000, are also presented, as are GMRT observations of H i in the direction of three sources, B1801−203, B1802−19...
متن کامل3-D Analytic Signal in the Interpretation of Total Magnetic Field Data at Low Magnetic Latitudes
The interpretation of magnetic field data at low magnetic latitudes is difficult because the vector nature of the magnetic field increases the complexity of anomalies from magnetic rocks. The most obvious approach to this problem is to reduce the data to the magnetic pole, where the presumably vertical magnetization vector will simplify observed anomalies. However, RTP requires special treatmen...
متن کاملSummertime low - ozone episodes at northern high latitudes
By Y. J. ORSOLINI1∗, H. ESKES2, G. HANSEN1, U.-P. HOPPE3, A. KYLLING1, E. KYRÖ4, J. NOTHOLT5, R. VAN DER A2 and P. VON DER GATHEN6 1Norwegian Institute for Air Research, Kjeller, Norway 2Royal Netherlands Meteorological Institute, De Bilt, the Netherlands 3Norwegian Defence Research Establishment, Kjeller, Norway 4Finnish Meteorological Institute, Sodankyla, Finland 5University of Bremen, Germa...
متن کاملA search for microquasar candidates at low galactic latitudes
Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very useful in trying to understand the accretion/ejection processes that take place near compact objects. However, the number of sources involved in such studies is still small. In an attempt to increase the number of known microquasars we have carried out a search for new Radio Emitting X-ray Binar...
متن کاملStructure of the Sagittarius dwarf galaxy at low Galactic latitudes
We report the detection of ∼1 500 RR Lyrae of Bailey type ab located in the Sagittarius dwarf galaxy (Sgr). These variables have been detected on two ESO Schmidt fields centred on (l,b)=(3.1,-7.1) and (6.6,10.8), covering an area of ∼50 deg. We present a surface density map of Sgr based on the spatial distribution of these RRab, allowing us to trace its structure in a region that was still almo...
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ژورنال
عنوان ژورنال: Journal of Earth System Science
سال: 1978
ISSN: 0253-4126,0973-774X
DOI: 10.1007/bf02839384