M. S. Yun
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Research Interests
M. S. Yun has a total of 13 co-authors. Here are the top co-authors by number of shared publications:
- Daniel Espada
Universidad de Granada
2 shared publications J. Sulentic
Department of Astronomy, University of Alabama, AL 35487, USA
2 shared publicationsL. Verdes-Montenegro
Instituto de Astrofisica de Andalucia, CSIC, Apdo. 3004, 18080 Granada, Spain
2 shared publicationsS. Leon
Instituto de Astrofisica de Andalucia, CSIC, Apdo. 3004, 18080 Granada, Spain
2 shared publicationsA. Bosma
Observatoire de Marseille, 2 place Le Verrier, 13248 Marseille Cedex 4, France
1 shared publicationE. Athanassoula
Observatoire de Marseille, 2 place Le Verrier, 13248 Marseille Cedex 4, France
1 shared publication
Latest Publications
- 7 October 2005
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 442 (2) , 455-459
The large asymmetric HI envelope of the isolated galaxy NGC 864 (CIG 96)
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics
- 7 October 2005
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 442 (2) , 455-459
The large asymmetric HI envelope of the isolated galaxy NGC 864 (CIG 96)
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics
- 1 January 2004
- Published by Cambridge University Press (CUP) in Symposium - International Astronomical Union
- Vol. 217, 220-221
A Reference Sample: ISM of the Most Isolated Galaxies
We are constructing the first complete unbiased control sample of the most isolated galaxies of the northern sky to serve as a template in the study of star formation and galaxy evolution in denser environments. Our goal is to compare and quantify the properties of different phases of the interstellar medium in this sample, as well as the level of star formation, both relevant parameters in the internal evolution of galaxies and strongly conditioned by the environment. To achieve this goal we are building a multiwavelength database for this sample to compare and quantify the properties of different phases of the ISM.
- 1 January 2004
- Published by Cambridge University Press (CUP) in Symposium - International Astronomical Union
- Vol. 217, 220-221
A Reference Sample: ISM of the Most Isolated Galaxies
We are constructing the first complete unbiased control sample of the most isolated galaxies of the northern sky to serve as a template in the study of star formation and galaxy evolution in denser environments. Our goal is to compare and quantify the properties of different phases of the interstellar medium in this sample, as well as the level of star formation, both relevant parameters in the internal evolution of galaxies and strongly conditioned by the environment. To achieve this goal we are building a multiwavelength database for this sample to compare and quantify the properties of different phases of the ISM.