Proje»En I Rtr

En I Rtr

There is a potential need for IR Astronomy in Turkey. Below are some examples to the subjects of interest.

In alphabetical (surname) order

Nazım Aksaker / Çukurova University - Department of Physics

Planetary nebulas and their formation; interstellar gas


Sinan Aliş / Istanbul University - Department of Astronomy and Space Sciences

Clusters of galaxies; brightest cluster galaxies; high red-shift galaxies


Şölen Balman / Middle East Technical University - Department of Physics

Infrared coronal emission in later stages of classical nova explosions; Cataclysmic Variables (CV): outer parts of the disks, spectroscopy of the secondary stars, etc.; infrared time series analysis and ellipsoidal oscillation analysis in Cataclysmic Variables and Low-mass X-ray Binaries; magnetic CVs


Selçuk Bilir / Istanbul University - Department of Astronomy and Space Sciences

IR surveying


Hakan Erkut / Istanbul Kültür University

Possibility of observing disks around isolated neutron stars in near- and mid-IR; planet formation in these supernova remnant disks


Ünal Ertan / Sabancı University

Disk structures around compact objects


Tolga Güver / University of Arizona, US

Searching for the IR components of isolated neutron stars, X-ray binaries, and magnetars; analysing the properties of interstellar medium; IR surveying


Emrah Kalemci / Sabancı University

Analysing the blackhole-jet systems in our Galaxy


Ümit Kızıloğlu / Middle East Technical University - Department of Physics

Disk structures of Be/X stars


Aybüke Küpçü Yoldaş / ESO, DE; Cambridge IoA, UK

Gamma-ray bursts (GRB) and host galaxies; galaxy formation and evolution


İlham Nasıroğlu / Çukurova University, Department of Physics

Investigating the possibility of a fast photo-polarimeter for point sources


Rennan Pekünlü / Ege University - Department of Astronomy and Space Sciences

Magnetic Cataclysmic Variables (MCVs)


Cahit Yeşilyaprak / Erzurum Atatürk University - Department of Physics

Atmospheres of red stars; relations between metal lines and mass loss; star-formation regions; IR surveying


Umut A. Yıldız / Leiden Observatory, Holland

Protostars in star-forming regions (SFRs) -- (far-IR, sub-mm)