On the period variation of the neglected W UMa-type binary system V714 monocerotis
Some new CCD times of the light minimum for a neglected W UMa-type binary star, V714 Monocerotis, observed in 2002 and 2003, are presented. By considering the general trend of the O - C variation, a plausible O - C curve was formed and a mean linear ephemeris was obtained. It was found that the peri...
Saved in:
Main Authors: | , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
2014
|
Online Access: | http://www.scopus.com/inward/record.url?eid=2-s2.0-3142676826&partnerID=40&md5=57ebf204a3a63c1be79bd9b54f1aab37 http://cmuir.cmu.ac.th/handle/6653943832/6976 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Institution: | Chiang Mai University |
Language: | English |
id |
th-cmuir.6653943832-6976 |
---|---|
record_format |
dspace |
spelling |
th-cmuir.6653943832-69762014-08-30T03:51:27Z On the period variation of the neglected W UMa-type binary system V714 monocerotis Qian S.-B. Soonthornthum B. Xiang F.-Y. Zhu L.-Y. He J.-J. Some new CCD times of the light minimum for a neglected W UMa-type binary star, V714 Monocerotis, observed in 2002 and 2003, are presented. By considering the general trend of the O - C variation, a plausible O - C curve was formed and a mean linear ephemeris was obtained. It was found that the period of the binary star shows a continuous decrease with rate of dP/dt = -1.48 × 10-7 d yr-1. In order to understand the evolutionary state of the binary system, new photometric and spectroscopic observations and a careful investigation on those data are required. 2014-08-30T03:51:27Z 2014-08-30T03:51:27Z 2004 Article 00046264 http://www.scopus.com/inward/record.url?eid=2-s2.0-3142676826&partnerID=40&md5=57ebf204a3a63c1be79bd9b54f1aab37 http://cmuir.cmu.ac.th/handle/6653943832/6976 English |
institution |
Chiang Mai University |
building |
Chiang Mai University Library |
country |
Thailand |
collection |
CMU Intellectual Repository |
language |
English |
description |
Some new CCD times of the light minimum for a neglected W UMa-type binary star, V714 Monocerotis, observed in 2002 and 2003, are presented. By considering the general trend of the O - C variation, a plausible O - C curve was formed and a mean linear ephemeris was obtained. It was found that the period of the binary star shows a continuous decrease with rate of dP/dt = -1.48 × 10-7 d yr-1. In order to understand the evolutionary state of the binary system, new photometric and spectroscopic observations and a careful investigation on those data are required. |
format |
Article |
author |
Qian S.-B. Soonthornthum B. Xiang F.-Y. Zhu L.-Y. He J.-J. |
spellingShingle |
Qian S.-B. Soonthornthum B. Xiang F.-Y. Zhu L.-Y. He J.-J. On the period variation of the neglected W UMa-type binary system V714 monocerotis |
author_facet |
Qian S.-B. Soonthornthum B. Xiang F.-Y. Zhu L.-Y. He J.-J. |
author_sort |
Qian S.-B. |
title |
On the period variation of the neglected W UMa-type binary system V714 monocerotis |
title_short |
On the period variation of the neglected W UMa-type binary system V714 monocerotis |
title_full |
On the period variation of the neglected W UMa-type binary system V714 monocerotis |
title_fullStr |
On the period variation of the neglected W UMa-type binary system V714 monocerotis |
title_full_unstemmed |
On the period variation of the neglected W UMa-type binary system V714 monocerotis |
title_sort |
on the period variation of the neglected w uma-type binary system v714 monocerotis |
publishDate |
2014 |
url |
http://www.scopus.com/inward/record.url?eid=2-s2.0-3142676826&partnerID=40&md5=57ebf204a3a63c1be79bd9b54f1aab37 http://cmuir.cmu.ac.th/handle/6653943832/6976 |
_version_ |
1681420714487316480 |