activity
19992009
most citedThe effect of violent star formation on the state of the molecular gas in M82

201 citations · 606 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2009★ 8 cited

The molecular gas content of the advanced S+E merger NGC 4441 - Evidence for an extended decoupled nuclear disc?

E. Juette, S. Aalto, S. Huettemeister

Mergers between a spiral and an elliptical (S+E mergers) are poorly studied so far despite the importance for galaxy evolution. NGC4441 is a nearby candidate for an advanced remnan…

astro-ph2004★ 35 cited

Stellar Disk Truncations: Where do we stand ?

M. Pohlen, J. E. Beckman, S. Huettemeister +3

In the light of several recent developments we revisit the phenomenon of galactic stellar disk truncations. Even 25 years since the first paper on outer breaks in the radial light…

astro-ph2001★ 130 cited

CN and HNC Line Emission in IR Luminous Galaxies

S. Aalto, A. G. Polatidis, S. Huttemeister +1

We have observed HNC 1-0, CN 1-0 and 2-1 line emission in a sample of 13 IR luminous (LIRGs, L_IR > 10E11 Lo) starburst and Seyfert galaxies. HNC 1-0 is detected in 9, CN 1-0 is de…

astro-ph2000★ 56 cited

The Interaction between the ISM and Star Formation in the Dwarf Starburst Galaxy NGC 4214

F. Walter, C. Taylor, S. Huettemeister +2

We present the first interferometric study of the molecular gas in the metal-poor dwarf starburst galaxy NGC 4214. Our map of the 12CO(1-0) emission, obtained at the OVRO millimete…

astro-ph2000★ 201 cited

The effect of violent star formation on the state of the molecular gas in M82

A. Weiss, N. Neininger, S. Huettemeister +1

We present the results of a high angular resolution, multi-transition analysis of the molecular gas in M82. The analysis is based on the two lowest transitions of 12CO and the grou…

astro-ph2000★ 80 cited

Warm H2 in the Galactic center region

N. J. Rodriguez-Fernandez, J. Martin-Pintado, A. Fuente +3

We present ISO observations of several H2 pure-rotational lines (from S(0) to S(5)) towards a sample of 16 molecular clouds distributed along the central ~ 500 pc of the Galaxy. We…