ON THE DISTANCE OF THE MAGELLANIC CLOUDS USING CEPHEID NIR AND OPTICAL–NIR PERIOD–WESENHEIT RELATIONS
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European Southern Observatory | Napoli | Munchen | Rome | The University of Tokyo | Astronomy | Institute of Astronomy | Italy | K. Genovali | L. Inno | C. D. Laney | Brigham Young University | F. Primas | School of Science | G. Bono | R. Buonanno | A. M. Piersimoni | Italy. | T. U. O. Tokyo | I. O. Astronomy | E. Observatory | School of Materials Science | M. Marconi | G. Bono | Romé | F. Primas | R. Buonanno | A. Piersimoni | L. Inno | M. Catone | M. Marconi | N. Matsunaga | F. Caputo | Universita' di Roma Tor Vergata | S. Z. O. A. D. Capodimonte | I. O. T. Physics | N. Matsunaga | Universita di Roma Tor Vergata | F. Caputo | Monte Porzio Catone | Teramo | Mitake | Kiso-machi | M. Romaniello Dipartimento di Fisica | Germany Kiso Observatory | Japan INAF--OAR | Italy INAF-Osservatorio Astronomico di Collurania | Italy Dept. of Physics | USA South African Astronomical Observatory | South Africa INAF-Osservatorio Astronomico di Capodimonte | Usa Uppsala Astronomical Observatory | K. Genovali | M. F. D. D. Fisica | Japan INAF--OAR | I. I. A. D. Collurania
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