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Collisional Debris as Laboratories to Study Star Formation

Boquien, M.; Duc, P.A.; Wu, Y.; Charmandaris, V.; Lisenfeld, U.; Braine, J.; Brinks, E.; Iglesias-Paramo, J.; Xi, C.K. (2009)

In this paper we address the question of whether star formation (SF) is driven by local processes or the large-scale environment. To do so, we investigate SF in collisional debris where the gravitational potential well and ...

VCC 2062: an old tidal dwarf galaxy in the Virgo cluster

Duc, P.A.; Braine, J.; Lisenfeld, U.; Brinks, E.; Boquien, M. (2007)

Polychromatic view of intergalactic star formation in NGC 5291

Boquien, M.; Duc, P.A.; Braine, J.; Brinks, E.; Lisenfeld, U.; Charmandaris, V. (2007)

Molecular and ionized gas in the tidal tail in Stephan's Quintet

Lisenfeld, U.; Braine, J.; Duc, P.A.; Brinks, E.; Charmandaris, V.; Leon, S. (2004-11)

Colliding molecular clouds in head-on galaxy collisions

Braine, J.; Lisenfeld, U.; Duc, P.A.; Brinks, E.; Charmandaris, V.; Leon, S. (2004-05)

Molecular Gas in the Intergalactic Medium of Stephan's Quintet

Lisenfeld, U.; Leon, S.; Braine, J.; Duc, P.A.; Charmandaris, V.; Brinks, E. (2003)

Molecular Gas in the Intergalactic Medium of Stephan's Quintet

Lisenfeld, U.; Leon, S.; Braine, J.; Duc, P.A.; Charmandaris, V.; Brinks, E. (Astronomical Society of the Pacific, 2003)

Abundant molecular gas in the intergalactic medium of Stephan's Quintet

Lisenfeld, U.; Braine, J.; Duc, P.A.; Leon, S.; Charmandaris, V.; Brinks, E. (2002-11)

Stephan's Quintet (SQ) is a system consisting of at least four interacting galaxies which is well known for its complex dynamical and star formation history. It possesses a rich intergalactic medium (IGM), where hydrogen ...

Star Formation in Tidal Dwarf Galaxies

Lisenfeld, U.; Braine, J.; Vallejo, O.; Duc, P.A.; Leon, S.; Brinks, E.; Charmandaris, V. (Astronomical Society of the Pacific, 2002)

Tidal Dwarf Galaxies (TDGs) are objects presently forming from gas that has been expelled from their parent galaxies during an interaction. We searched for CO emission in a sample of 11 TDGs, of which 8 were detected. The ...