Calculating space velocities (U, V, and W)‎ for stars in the halo of our galaxy

Other Title(s)

حساب السرع الفضائية (U, V, and W)‎ لعدد من النجوم في هالة مجرتنا

Author

Abd al-Latif, Abbas

Source

Iraqi Journal of Science

Issue

Vol. 53, Issue 4 (31 Dec. 2012), pp.916-923, 8 p.

Publisher

University of Baghdad College of Science

Publication Date

2012-12-31

Country of Publication

Iraq

No. of Pages

8

Main Subjects

Astronomy

Abstract AR

السرع الفضائية (and W،V،U) لعدد من النجوم في هالة مجرتنا قد تم حسابها باختيار نجوم ذات أطياف (and K،G،A) على مسافة تقرب من عشرة فراسخ من الشمس.

لقد وجدنا أن بعض هذه النجوم تمثل مجموعة مترابطة.

نجوم هذه المجموعة متشابهة غي الحركة الثلاثية الأبعاد، و أنها في المجموعة الشمسية المجاورة.

لقد بينت النتائج أن سرع هذه النجوم مترابطة فيما بينها.

Abstract EN

Space velocities (U, V, and W)for many stars in the halo of our galaxy were calculated by choosing A, G and K spectral type stars at a distance nearly 10 pc.

It was found that some of these stars represent a Local Association group (kinematic stream), the stars of this group are sharing in similar 3-D kinematic motion in the galaxy, in the solar neighborhood.

The results displayed that these velocities are in a good correlation with each other.

American Psychological Association (APA)

Abd al-Latif, Abbas. 2012. Calculating space velocities (U, V, and W) for stars in the halo of our galaxy. Iraqi Journal of Science،Vol. 53, no. 4, pp.916-923.
https://search.emarefa.net/detail/BIM-323391

Modern Language Association (MLA)

Abd al-Latif, Abbas. Calculating space velocities (U, V, and W) for stars in the halo of our galaxy. Iraqi Journal of Science Vol. 53, no. 4 (2012), pp.916-923.
https://search.emarefa.net/detail/BIM-323391

American Medical Association (AMA)

Abd al-Latif, Abbas. Calculating space velocities (U, V, and W) for stars in the halo of our galaxy. Iraqi Journal of Science. 2012. Vol. 53, no. 4, pp.916-923.
https://search.emarefa.net/detail/BIM-323391

Data Type

Journal Articles

Language

English

Notes

Includes bibliographical references : p. 923

Record ID

BIM-323391