Relevant bibliographies by topics / Mira variable stars

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Mira variable stars'

Author: Grafiati
Published: 4 June 2021
Last updated: 20 February 2023

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Mira variable stars.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Mira variable stars"

1

Nakagawa, Akiharu, Tomoharu Kurayama, Toshihiro Omodaka, Tatsuya Kamezaki, Yoshiro Nishida, and Makoto Matsui. "The period–luminosity relation of Mira variable stars." Proceedings of the International Astronomical Union 8, S289 (2012): 217. http://dx.doi.org/10.1017/s1743921312021412.

Full text
Abstract:
AbstractWe use astrometry to measure the distances to Galactic Mira variable stars. Our purpose is to determine a precise period–luminosity relation (PLR). At present, we do not have a precise PLR for Galactic Mira stars because of the large uncertainties affecting their distance estimates. To reduce the uncertainties, we adopted the Very Long Baseline Interferometry method and measured annual parallaxes of Mira variable stars with VERA. In addition to our previous results, we obtained three new distances for Mira variable stars. Based on our observations, the typical uncertainty in a given di
APA, Harvard, Vancouver, ISO, and other styles
2

Castelaz, Michael W., Donald G. Luttermoser, Daniel B. Caton, and Robert A. Piontek. "Phase-dependent Spectroscopy of Mira Variable Stars." Astronomical Journal 120, no. 5 (2000): 2627–37. http://dx.doi.org/10.1086/316837.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Luttermoser, Donald G., George H. Bowen, and Lee Anne Willson. "NLTE Synthetic Spectra of Mira-Type Variable Stars." International Astronomical Union Colloquium 139 (1993): 207. http://dx.doi.org/10.1017/s025292110011735x.

Full text
Abstract:
AbstractWe present NLTE radiative transfer in hydrodynamic models representative of Mira-type variable stars. Calculations were carried out with the PANDORA code of the Bowen models using a snapshot approximation.
APA, Harvard, Vancouver, ISO, and other styles
4

Iwanek, Patryk, Igor Soszyński, Szymon Kozłowski, et al. "The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way." Astrophysical Journal Supplement Series 260, no. 2 (2022): 46. http://dx.doi.org/10.3847/1538-4365/ac6676.

Full text
Abstract:
Abstract We present a collection of 65,981 Mira-type variable stars found in the Optical Gravitational Lensing Experiment (OGLE) project database. Two-thirds of our sample (40,356 objects) are located in the Galactic bulge fields, whereas 25,625 stars are in the Galactic disk. The vast majority of the collection (47,532 objects) comprises new discoveries. We provide basic observational parameters of the Mira variables: equatorial coordinates, pulsation periods, I-band and V-band mean magnitudes, I-band brightness amplitudes, and identifications in other catalogs of variable stars. We also prov
APA, Harvard, Vancouver, ISO, and other styles
5

Esipov, V. F., M. I. Pashchenko, G. M. Rudnitskij, et al. "Multiwavelength Studies of Mira Ceti-type Variable Stars." Symposium - International Astronomical Union 191 (1999): 201–6. http://dx.doi.org/10.1017/s0074180900203082.

Full text
Abstract:
Since 1994, observations of a sample of about 20 Mira Ceti-type and semiregular variables have been carried out in three spectral ranges: radio (H2O maser line λ = 1.35 cm), optical (spectroscopy and UBV photometry) and infrared (JHKLM photometry). Time series of the Hα emission intensity and H2O line flux, covering several periods of the stars, have been obtained. Correlation of the intensity variations of the H2O maser with optical variability in the maser stars RR Aql, U Ori, VX Sgr and others was confirmed. One of the most interesting results is the flare of the H2O maser emission in R Leo
APA, Harvard, Vancouver, ISO, and other styles
6

Little, S. J., та I. R. Little-Marenin. "The 8-22μm Excess in Carbon Stars From IRAS LRS Spectra". International Astronomical Union Colloquium 106 (1989): 402. http://dx.doi.org/10.1017/s0252921100063429.

Full text
Abstract:
We have measured the excess IR emission from carbon mira and SR variable stars from IRAS LRS spectra. The 8-22μm excess is defined as the ratio of flux above a 2500K energy distribution fit to the LRS spectrum at about 8μm. The carbon star LRS spectra show both emission and absorption features, which are incorporated into our 8-22pm excess. The most prominent feature in carbon stars is the 11.2μm SiC dust emission feature extending from 10μm to 13.8 μm. We observe another emission feature of unknown origin which peaks between 8.4-8.7μm. The SiC emission feature is occasionally blended on the r
APA, Harvard, Vancouver, ISO, and other styles
7

Rudnitskij, Georgij M. "Molecular Masers in Variable Stars." Publications of the Astronomical Society of Australia 19, no. 4 (2002): 499–504. http://dx.doi.org/10.1071/as02018.

Full text
Abstract:
AbstractWhen a star with a mass of one to a few solar masses enters the red giant stage of its evolution, the radius of its atmosphere reaches several astronomical units. Pulsational instability is typical for this stage. Most stars become Mira-type or semiregular variables with light cycles of a few hundred days. Red giants lose mass at a rate M = 10−7−10−5M⊙ yr−1. Extensive gas–dust circumstellar envelopes form. These envelopes contain various molecular species. Some of these molecules (OH, H2O, SiO, HCN) manifest themselves in maser radio emission. Data on the H2O maser variability and its
APA, Harvard, Vancouver, ISO, and other styles
8

Mennessier, Marie-Odile, Hichame Boughaleb, and Janet A. Mattei. "Comparison of Mean Light Curve Parameters of M, S and C Mira and Semi-Regular Variable Stars Using 75 Years of AAVSO Data." Symposium - International Astronomical Union 177 (2000): 165–70. http://dx.doi.org/10.1017/s0074180900002370.

Full text
Abstract:
Using 75 years of AAVSO data, mean light curve parameters of a sample of 350 long-period M, S and C Mira and semi-regular variable stars have been investigated. We compare M, S and C Mira and semi-regular stars, present a classification of the light curves of LPVs and give discriminant parameters.
APA, Harvard, Vancouver, ISO, and other styles
9

Kudashkina, L. S., and I. L. Andronov. "Multiharmonic analysis of Mira-type stars." Symposium - International Astronomical Union 180 (1997): 353. http://dx.doi.org/10.1017/s0074180900131286.

Full text
Abstract:
The shapes of light curves of Mira-type variable stars are analyzed by using the multi–harmonic fit (Andronov 1994). The light curves of 63 stars best covered by the AAVSO observations and published by Mattei (1978) were used. Some correlations between the characteristics of the mean light curves were found.
APA, Harvard, Vancouver, ISO, and other styles
10

Shibahashi, Hiromoto. "Implication of a P-L Relation of Mira Variables." International Astronomical Union Colloquium 139 (1993): 103. http://dx.doi.org/10.1017/s0252921100117014.

Full text
Abstract:
Feast et al. (1989) obtained observationally a period-luminosity (P-L) relation of Mira variables in LMC. Basically, fundamental periods of stellar pulsation should be determined by two quantities —a mass and a radius of the star. The existence of a P-L relation implies a special condition that reduces a function of two variables into a function of only a single variable. Though the AGB appears as a thin line in the HR diagram like the Cepheid instability strip, it is an “asymptotically” merged line of evolutionary tracks of stars in a range of about 0.5-3 solar masses. This fact means that th
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Mira variable stars"

1

Ireland, Michael James. "Optical Interferometry and Mira Variable Stars." University of Sydney. Physics, 2005. http://hdl.handle.net/2123/721.

Full text
Abstract:
This thesis describes the development of a red tip/tilt and fringe detection system at the Sydney University Stellar Interferometer (SUSI), modelling the instrumental performance and effects of seeing at SUSI, making observations of Mira variable stars and finally modelling the atmospheres of Mira variables with physically self-consistent models. The new SUSI tip/tilt system is based around a CCD detector and has been successfully used to both track the majority of tip/tilt power in median seeing at an R magnitude of 4.5, and to provide seeing measures for post processing. The new fringe-det
APA, Harvard, Vancouver, ISO, and other styles
2

Ireland, Michael. "Optical interferometry and Mira variable stars /." Connect to full text, 2005. http://hdl.handle.net/2123/721.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Friedman, Vanessa Ann. "Identifying Long Period Variable (LPV) Stars Using Images from the Stardial Observatory." Thesis, The University of Arizona, 2009. http://hdl.handle.net/10150/193423.

Full text
Abstract:
The study of variable stars is extremely important to the astronomical field of scientific research. Variable stars must be methodically studied, usually by amateur astronomers over a long period of time, in order to provide professional astronomers important data that allows them to further analyze variable star behavior.Variable stars are unique because their pulsation produces visible changes in luminosity. This pulsation allows amateur astronomers to visually observe and identify variable stars. This type of research and study is special because amateurs can make a real contribution to the
APA, Harvard, Vancouver, ISO, and other styles
4

Caddy, Robert V. "Time Series Photometry of the Symbiotic Star V1835 Aql and New Variable Stars in Aquila." Bowling Green State University / OhioLINK, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1525438143057776.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Neilson, Hilding, Richard Ignace, Beverly Smith, Gary Henson, and Alyssa Adams. "Evidence of a Mira-like tail and bow shock about the semi-regular variable V CVn from four decades of polarization measurements." Digital Commons @ East Tennessee State University, 2014. https://dc.etsu.edu/etsu-works/6233.

Full text
Abstract:
Polarization is a powerful tool for understanding stellar atmospheres and circumstellar environments. Mira and semi-regular variable stars have been observed for decades and some are known to be polarimetrically variable, however, the semi-regular variable V Canes Venatici displays an unusually large, unexplained amount of polarization. We present ten years of optical polarization observations obtained with the HPOL instrument, supplemented by published observations spanning a total interval of about forty years for V CVn. We find that V CVn shows large polarization variations ranging from 1 -
APA, Harvard, Vancouver, ISO, and other styles
6

Cardona, Velasquez Gustavo Adolfo. "Properties of Bright Variable Stars in Unusual Metal Rich Cluster NGC 6388." Bowling Green State University / OhioLINK, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1308577583.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Kager, Elisabeth. "Pulsation Properties of Long Period Variable Stars in Globular Cluster NGC 6553." Bowling Green State University / OhioLINK, 2010. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1277148078.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Aljassim, Mohammad A. "A 6-Year Study of Long Period Variable Stars in the Globular Cluster NGC 6388." Bowling Green State University / OhioLINK, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1499442952467274.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Abbas, Mohamad. "A search for Long-Period Variable Stars in the Globular Cluster NGC 6496." Bowling Green State University / OhioLINK, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1308597257.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Tuthill, Peter George. "Imaging stars through the atmosphere." Thesis, University of Cambridge, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.337414.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Books on the topic "Mira variable stars"

1

United States. National Aeronautics and Space Administration., ed. Final report to the National Aeronautics and Space Administration concerning the Astrophysical Data Program entitled, The chromosphere/shock dilemma of non-Mira, late-type variable stars: NASA grant number NAG 5-2830 : report covering the period, 12/15/94-12/14/96. National Aeronautics and Space Administration, 1997.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
2

United States. National Aeronautics and Space Administration., ed. Final report to the National Aeronautics and Space Administration concerning the Astrophysical Data Program entitled, The chromosphere/shock dilemma of non-Mira, late-type variable stars: NASA grant number NAG 5-2830 : report covering the period, 12/15/94-12/14/96. National Aeronautics and Space Administration, 1997.

Find full text
APA, Harvard, Vancouver, ISO, and other styles

Book chapters on the topic "Mira variable stars"

1

Yi, Jiyune, R. S. Booth, and J. E. Conway. "Phase Dependence of 43 GHz SiO Masers in the Mira Variable TX Cam." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_68.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Sato, Koichi, Masanori Yoshizawa, Jun Nishikawa, Naoko Ohishi, and Takayuki Kotani. "Mira Project and the Observations of Mira Variables." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_91.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Zijlstra, Albert A., Mikako Matsuura, and Timothy R. Bedding. "Period Evolution in Mira Variables." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_13.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Groenewegen, M. A. T., P. A. Whitelock, C. H. Smith, and F. Kerschbaum. "Dust Shells around Carbon Mira Variables." In Dust and Molecules in Evolved Stars. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-017-1307-8_11.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Vardya, M. S. "Some Properties of S Mira Variables." In Cool Stars with Excesses of Heavy Elements. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5325-3_14.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Feast, Michael. "The Galactic Kinematics of Mira Variables." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_12.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Hinkle, Kenneth H., and Werner W. G. Scharlach. "Carbon Isotope Ratios in Oxygen Rich Mira and SRa Variables." In Cool Stars with Excesses of Heavy Elements. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5325-3_33.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Humphreys, E. M. L., M. D. Gray, D. Field, J. A. Yates, and G. Bowen. "A Model for the Variability of SiO Masers in Mira Variables." In Dust and Molecules in Evolved Stars. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-017-1307-8_31.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Onaka, Takashi, Teije de Jong, and Issei Yamamura. "Time Variation of Mid-Infrared Spectra of M-Type Mira Variables." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_62.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Kurayama, Tomoharu, and Tetsuo Sasao. "Annual Parallax Measurements of Mira-Type Variables with Phase-Reference VLBI Observation." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_50.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Mira variable stars"

1

Karovicova, Iva, Markus Wittkowski, David A. Boboltz, Michael Scholz, and Eric Stempels. "Coordinated AMBER and MIDI observations of the Mira variable RR Aql." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099285.

Full text
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Mira variable stars' for particular source types:
Journal articles
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography