Поиск по публикациям

Astrometry of the Galactic Miras and LPVs with a Japanese VLBI Array “Vera”

A. Nakagawa, T. Kurayama, G. Orosz, VERA Project

Труды ИПА РАН, вып. 40, 28–33 (2017)

Ключевые слова: Variable star, VLBI, Astrometry

Информация о статье Текст статьи

Аннотация

A relation between pulsation periods and magnitudes (PL-relation) of the Galactic long period variable (LPVs) is studied based on VLBI observations. Calibra tion of the PL-relation applied to the Galactic LPVs is our scientific aim. From 2004, we have been conducting astrometric VLBI observations towards dozens of Mira and semiregular variables to measure their parallaxes. Current result of our ongoing study is presented. As a future plan, we started a study of mid-infrared PL-relations applied to OH/IR stars with period longer than ∼1000 days. We mention a contribution to the study of Galactic kinematics from our research of OH/IR stars.

Цитирование

Текст
Бибтех
RIS
A. Nakagawa, T. Kurayama, G. Orosz, VERA Project. Astrometry of the Galactic Miras and LPVs with a Japanese VLBI Array “Vera” // Труды ИПА РАН. — 2017. — Вып. 40. — С. 28–33. @article{nakagawa2017, abstract = {A relation between pulsation periods and magnitudes (PL-relation) of the Galactic long period variable (LPVs) is studied based on VLBI observations. Calibra tion of the PL-relation applied to the Galactic LPVs is our scientific aim. From 2004, we have been conducting astrometric VLBI observations towards dozens of Mira and semiregular variables to measure their parallaxes. Current result of our ongoing study is presented. As a future plan, we started a study of mid-infrared PL-relations applied to OH/IR stars with period longer than ∼1000 days. We mention a contribution to the study of Galactic kinematics from our research of OH/IR stars.}, author = {A. Nakagawa and T. Kurayama and G. Orosz and VERA Project}, issue = {40}, journal = {Труды ИПА РАН}, keyword = {Variable star, VLBI, Astrometry}, pages = {28--33}, title = {Astrometry of the Galactic Miras and LPVs with a Japanese VLBI Array “Vera”}, url = {http://iaaras.ru/library/paper/1675/}, year = {2017} } TY - JOUR TI - Astrometry of the Galactic Miras and LPVs with a Japanese VLBI Array “Vera” AU - Nakagawa, A. AU - Kurayama, T. AU - Orosz, G. AU - Project, VERA PY - 2017 T2 - Труды ИПА РАН IS - 40 SP - 28 AB - A relation between pulsation periods and magnitudes (PL-relation) of the Galactic long period variable (LPVs) is studied based on VLBI observations. Calibra tion of the PL-relation applied to the Galactic LPVs is our scientific aim. From 2004, we have been conducting astrometric VLBI observations towards dozens of Mira and semiregular variables to measure their parallaxes. Current result of our ongoing study is presented. As a future plan, we started a study of mid- infrared PL-relations applied to OH/IR stars with period longer than ∼1000 days. We mention a contribution to the study of Galactic kinematics from our research of OH/IR stars. UR - http://iaaras.ru/library/paper/1675/ ER -