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Supershells in the M33 Galaxy

  • A. Leščinskaitė EMAIL logo , R. Stonkutė and V. Vansevičius
Published/Copyright: February 18, 2017
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Open Astronomy
From the journal Open Astronomy Volume 24 Issue 3

Received: 2015-10-12
Accepted: 2015-10-30
Published Online: 2017-2-18
Published in Print: 2015-9-1

© 2015 A. Leščinskaitė et al., published by De Gruyter Open

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  1. Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
  2. Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3
  3. Optics for Nano-Satellite X-Ray Monitor
  4. Observational Data and Orbits of the Asteroids Discovered at the Baldone Observatory in 2008–2013
  5. On the Pseudo Phase-space Density of Dark Matter Haloes and the Universality of Density Profiles
  6. Baryon Physics and the Missing Satellites Problem
  7. A Young Star Cluster in the Leo a Galaxy
  8. Supershells in the M33 Galaxy
  9. Structural Parameters of Star Clusters: Signal to Noise Effects
  10. Artificial Star Test for Crowded Field CCD Photometry
  11. Ultraviolet and Infrared Correlation Studies in Orion
  12. Ultraviolet Spectroscopic Investigation of HU Aqr and AN UMa with the Data from HST and IUE
https://doi.org/10.1515/astro-2017-0230
Keywords for this article
galaxies: individual (M 33); galaxies: ISM: supershells
Creative Commons
BY-NC-ND 3.0

Articles in the same Issue

  1. Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
  2. Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3
  3. Optics for Nano-Satellite X-Ray Monitor
  4. Observational Data and Orbits of the Asteroids Discovered at the Baldone Observatory in 2008–2013
  5. On the Pseudo Phase-space Density of Dark Matter Haloes and the Universality of Density Profiles
  6. Baryon Physics and the Missing Satellites Problem
  7. A Young Star Cluster in the Leo a Galaxy
  8. Supershells in the M33 Galaxy
  9. Structural Parameters of Star Clusters: Signal to Noise Effects
  10. Artificial Star Test for Crowded Field CCD Photometry
  11. Ultraviolet and Infrared Correlation Studies in Orion
  12. Ultraviolet Spectroscopic Investigation of HU Aqr and AN UMa with the Data from HST and IUE
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