SIMBAD references

2014ApJ...796...89S - Astrophys. J., 796, 89 (2014/December-1)

Tracing ram-pressure stripping with warm molecular hydrogen emission.


Abstract (from CDS):

We use the Spitzer Infrared Spectrograph to study four infalling cluster galaxies with signatures of ongoing ram-pressure stripping. H2 emission is detected in all four, and two show extraplanar H2emission. The emission usually has a warm (T ∼ 115-160 K) and a hot (T ∼ 400-600 K) component that is approximately two orders of magnitude less massive than the warm one. The warm component column densities are typically 1019 to 1020/cm2 with masses of 106 to 108 M. The warm H2is anomalously bright compared with normal star-forming galaxies and therefore may be excited by ram-pressure. In the case of CGCG 97-073, the H2is offset from the majority of star formation along the direction of the galaxy's motion in the cluster, suggesting that it is forming in the ram-pressure wake of the galaxy. Another galaxy, NGC 4522, exhibits a warm H2tail approximately 4 kpc in length. These results support the hypothesis that H2within these galaxies is shock-heated from the interaction with the intracluster medium. Stripping of dust is also a common feature of the galaxies. For NGC 4522, where the distribution of dust at 8 µm is well resolved, knots and ripples demonstrate the turbulent nature of the stripping process. The Hα and 24 µm luminosities show that most of the galaxies have star-formation rates comparable to similar mass counterparts in the field. Finally, we suggest a possible evolutionary sequence primarily related to the strength of ram-pressure that a galaxy experiences to explain the varied results observed in our sample.

Abstract Copyright:

Journal keyword(s): galaxies: clusters: intracluster medium - galaxies: evolution - galaxies: ISM - infrared: galaxies

Simbad objects: 15

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2014ApJ...796...89S and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact