IPM Positions

Resident Researcher, School of Astronomy

Research Interests

Microlensing structure formation

Research Activities

Kepler satellite provides a high accuracy data and can be used to detect acctivity of stars. In this work we are giong to study acctivity of stars with the data set.

Present Research Project at IPM

Activity of stars with kepler data

Related Papers

1.	H. Goodarzi, A. Mehrabi, H. Khosroshahi and H. He Flare Activity and Magnetic Feature Analysis of the Flare Stars. II. Subgiant Branch Astrophysical Journal 906 (2021),   [abstract] Code: IPM/A-2020/31

2.	H. Goodarzi, A. Mehrabi, H. khosroshahi and H. He Flare Activity and Magnetic Feature Analysis of the Flare Stars Astrophysical Journal Supplement Series 244 (2019),   [abstract] Code: IPM/A-2019/21

3.	A. Mehrabi and H. He Magnetic activity properties of M-type kepler stars ELSEVIER 66 (2019), 31-39  [abstract] Code: IPM/A-2018/33

4.	H. He, H. Wang, M. Zhang, A. Mehrabi, Y. Yan and D. Yun Phase difference between long-term magnetic feature activity and flare activity of solar-type stars IAU 13 (2018), 217-220  [abstract] Code: IPM/A-2018/35

5.	H. He, H. Wang, M. Zhang, A. Mehrabi, Y. Yan and D. Yun Activity Analyses for Solar-type Stars Observed with Kepler. II. Magnetic Feature versus Flare Activity Astrophysical Journal 236 (2018),   [abstract] Code: IPM/A-2018/34

6.	T. Naderi, A. Mehrabi and S. Rahvar Primordial black hole detection through diffractive microlensing Int. J. Mod. Phys. D 97 (2018),   [abstract] Code: IPM/A-2018/20

7.	A. Mehrabi, H. He and H. Khosroshahi MAGNETIC ACTIVITY ANALYSIS FOR A SAMPLE OF G-TYPE MAIN SEQUENCE KEPLER TARGETS Astrophysical Journal 834 (2017),   [abstract] Code: IPM/A-2016/30