Dynamics of blue compact galaxies, as revealed by their Hα velocity fields - II. Mass models and the starburst triggering mechanism
A&A, 374 3 (2001) 800-823
Published online: 2001-08-15
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Integral Field Spectroscopy of Blue Compact Dwarf Galaxies
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https://doi.org/10.1086/528785
The escape of Lyman photons from a young starburst: the case of Haro 11
M. Hayes, G. Ostlin, H. Atek, et al.Monthly Notices of the Royal Astronomical Society 382 (4) 1465 (2007)
https://doi.org/10.1111/j.1365-2966.2007.12482.x
The Nature of Nearby Counterparts to Intermediate‐Redshift Luminous Compact Blue Galaxies. III. Interferometric Observations of Neutral Atomic and Molecular Gas
C. A. Garland, D. J. Pisano, J. P. Williams, et al.The Astrophysical Journal 671 (1) 310 (2007)
https://doi.org/10.1086/522514
Dynamical masses of two young globular clusters in the blue compact galaxy ESO 338–IG04
G. Östlin, R. J. Cumming and N. BergvallAstronomy & Astrophysics 461 (2) 471 (2007)
https://doi.org/10.1051/0004-6361:20054461
Star-gas decoupling and a non-rotating stellar core in He 2-10
T. Marquart, K. Fathi, G. Östlin, et al.Astronomy & Astrophysics 474 (1) L9 (2007)
https://doi.org/10.1051/0004-6361:20078142
Feedback in the Local Lyman‐break Galaxy Analog Haro 11 as Probed by Far‐Ultraviolet and X‐Ray Observations
J. P. Grimes, T. Heckman, D. Strickland, et al.The Astrophysical Journal 668 (2) 891 (2007)
https://doi.org/10.1086/521353
3D spectroscopy with VLT/GIRAFFE
M. Puech, F. Hammer, H. Flores, G. Östlin and T. MarquartAstronomy & Astrophysics 455 (1) 119 (2006)
https://doi.org/10.1051/0004-6361:20054218
The Red Halo Phenomenon
E. Zackrisson, N. Bergvall, G. Ostlin, G. Micheva and M. LeksellThe Astrophysical Journal 650 (2) 812 (2006)
https://doi.org/10.1086/506928
First detection of Lyman continuum escape from a local starburst galaxy
N. Bergvall, E. Zackrisson, B.-G. Andersson, et al.Astronomy & Astrophysics 448 (2) 513 (2006)
https://doi.org/10.1051/0004-6361:20053788
Study of DDO 68: nearest candidate for a young galaxy?
S. A. Pustilnik, A. Y. Kniazev and A. G. PramskijAstronomy & Astrophysics 443 (1) 91 (2005)
https://doi.org/10.1051/0004-6361:20053102
Did most present-day spirals form during the last 8 Gyr?
F. Hammer, H. Flores, D. Elbaz, et al.Astronomy & Astrophysics 430 (1) 115 (2005)
https://doi.org/10.1051/0004-6361:20041471