Published April 1, 2016 | Version v1
Journal article Metadata-only

Colour relations for Mira and Semiregular (SR) type stars

Creators

  • 1. Atatürk University, Science Faculty, Department of Physics, Erzurum (Turkey)
  • 2. Atatürk University, Science Faculty, Department of Astronomy and Astrophysics, Erzurum (Turkey)

Description

In this study, the period-colour relations, the colour-colour relations and the effective temperature were examined for Semiregular (SR) and Mira type variable stars. SR variables show an obvious period-colour relations, especially in infrared (IR). There are differences between SR and Mira type variable stars with respect to their colour relations. It has been thought that these differencies are caused by their mass loss rates and their effective temperatures. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/707/1/012044

Additional details

Identifiers

DOI
10.1088/1742-6596/707/1/012044;

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
707
Journal Issue
1
Journal Page Range
[4 p.]
ISSN
1742-6596

Conference

Title
International physics conference at the Anatolian Peak
Acronym
IPCAP2016
Dates
25-27 Feb 2016
Place
Erzurum (Turkey)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
49005721
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ASTROPHYSICS; COLOR; INFRARED RADIATION; MASS TRANSFER; STELLAR WINDS; TEMPERATURE DEPENDENCE; VARIABLE STARS
Descriptors DEC
ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; PHYSICS; RADIATIONS; STARS; STELLAR ACTIVITY