12CO(J=3→2) detections in bulges of low surface brightness galaxies with APEX
نویسندگان
چکیده
منابع مشابه
Co Detections of Edge-on Low Surface Brightness Galaxies
We have obtained deep CO(1-0) observations of 8 nearby, edge-on, low surface brightness (LSB) spiral galaxies using the NRAO 12-m telescope. We report detections of 3 of our targets at > 4σ level as well as one marginal (∼ 3σ) detection. These are among the first direct detections of molecular gas in late-type, LSB spirals. Using a Galactic CO-to-H2 conversion factor, we derive MH2 ∼ 1.4 − 3.5 ...
متن کاملDetections of CO in Late-Type, Low Surface Brightness Spiral Galaxies
Using the IRAM 30-m telescope, we have obtained 12CO J=1-0 and 2-1 spectral line observations toward the nuclear regions of 15 edge-on, low surface brightness (LSB) spiral galaxies. Our sample comprises extreme late-type LSB spirals with disk-dominated morphologies and rotational velocities Vrot <∼120 km s −1. We report detections of four galaxies in at least one transition ( >∼5σ); for the rem...
متن کاملMassive Disks in Low Surface Brightness Galaxies
An update of the set of low surface brightness galaxies is presented which can be used to set constraints on the otherwise ambiguous decompositions of their rotation curves into contributions due to the various components of the galaxies. The selected galaxies show all clear spiral structure and arguments of density wave theory of galactic spiral arms are used to estimate the masses of the gala...
متن کاملThe environment of Low Surface Brightness Galaxies
Using the Early Data Release of the Sloan Digital Sky Survey (SDSS) we investigated the clustering properties of Low Surface Brightness (LSB) galaxies in comparison to normal, High Surface Brightness (HSB) galaxies. We selected LSB galaxies and HSB galaxies with well measured redshifts from the SDSS data base and performed three-dimensional neighbour counting analysis within spheres of radii be...
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ژورنال
عنوان ژورنال: Proceedings of the International Astronomical Union
سال: 2007
ISSN: 1743-9213,1743-9221
DOI: 10.1017/s1743921308017626