Search Results - "Saygac, A. T."

Young Stellar Objects in the Massive Star-forming Regions W51 and W43 by Saral, G., Hora, J. L., Audard, M., Koenig, X. P., Martínez-Galarza, J. R., Motte, F., Nguyen-Luong, Q., Saygac, A. T., Smith, H. A.

“…We present the results of our investigation of the star-forming complexes W51 and W43, two of the brightest in the first Galactic quadrant. In order to…”
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YOUNG STELLAR OBJECTS IN THE MASSIVE STAR-FORMING REGION W49 by Saral, G., Hora, J. L., Willis, S. E., Koenig, X. P., Gutermuth, R. A., Saygac, A. T.

“…ABSTRACT We present the initial results of our investigation of the star-forming complex W49, one of the youngest and most luminous massive star-forming…”
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ERRATUM: "YOUNG STELLAR OBJECTS IN THE MASSIVE STAR FORMING REGION W49" (2015, ApJ, 813, 25) by Saral, G., Hora, J. L., Willis, S. E., Koenig, X. P., Gutermuth, R. A., Saygac, A. T.

“…[This corrects the article PMC7489494.]…”
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Archival HST study of novae. I. The Seyfert galaxy NGC 3627 by Alis, S., Saygaç, A.T.

“…► We examine the nova rate in the NGC 3627. ► This is the first attempt to determine the nova rate in this system. ► Four novae is found. ► The nova rate of…”
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UBV Photometry of the Massive Eclipsing Binary TT Aur by Özdemir, S., Ak, H., Tanriver, M., Gülseçen, H., Gülseçen, S., Saygaç, A. T., Budding, E., Demircan, O.

“…UBV observations of the massive binary system TT Aur were carried out mainly at theTurkish National Observatory (TUG). These observations, together with IUE…”
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Generation of nonlinear magnetic flux tube wave energies in Procyon A by Fawzy, D E, Saygac, A T, Stȩpień, K

“…Abstract The aim of the current study is the computation of the magnetic flux tube wave energies and fluxes generated in the convection zone of Procyon A. This…”
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Young Stellar Objects in the Massive Star-Forming Regions W51 and W43 by Saral, G, Hora, J. L, Audard, M, Koenig, X. P, Martínez-Galarza, J. R, Motte, F, Nguyen-Luong, Q, Saygac, A. T, Smith, H. A

“…We present the results of our investigation of the star-forming complexes W51 and W43, two of the brightest in the first Galactic quadrant. In order to…”
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Optical identification and follow-up observations of SRGA J213151.5+491400 -- a new magnetic cataclysmic variable discovered with SRG Observatory by Balman, Ş, Khamitov, I, Kolbin, A, Çalışkan, E. Aktekin, Bikmaev, I, Özdönmez, A, Burenin, R, Kılıç, Y, Esenoğlu, H. H, Yelkenci, K. F, Çamurdan, D. Zengin, Gilfanov, M, Nasıroğlu, I, Sonbaş, E, Gabdeev, M, Irtuganov, E, Saygaç, A. T, Nikolaeva, E, Sakhibullin, N, Er, H, Sazonov, S, Medvedev, P, Güver, T, Fişek, S

“…We report results of optical identification and multi-wavelength study of a new polar-type magnetic cataclysmic variable (MCV), SRGA J213151.5+491400,…”
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Optical and Ultraviolet Spectroscopy of VW Hydri by Saygac, A. Talat

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Photometry of the Massive Eclipsing Binary TT Aur by H. Ak, M. Tanriver, H. Gülseçen, S. Gülseçen, A. T. Saygaç, E. Budding, O. Demircan

“…Received 2000 May 3, accepted 2001 April 20 UBV observations of the massive binary system TT Aur were carried out mainly at theTurkish National Observatory…”
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