5 pages, 1 PostScript figure. To be published in the proceedings of the Zermatt 2010 conference: ``Conditions and impact of star formation: New results with Herschel and beyond''. Uses EAS LaTeX macros.We show that the XCO factor, which converts the CO luminosity into the column density of molecular hydrogen has similar values for dense, fully molecular gas and for diffuse, partially molecular gas. We discuss the reasons of this coincidence and the consequences for the understanding of the interstellar medium
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We have used archival far-ultraviolet spectra from observations made by HST/STIS and FUSE to determi...
International audienceContext: Most diffuse clouds are only known as kinematic features in absorptio...
5 pages, 1 PostScript figure. To be published in the proceedings of the Zermatt 2010 conference: ``C...
5 pages, 1 PostScript figure. To be published in the proceedings of the Zermatt 2010 conference: ``C...
Accepted to A&A 8 May 2010International audienceAims: We wish to separate and quantify the CO lumino...
Accepted to A&A 8 May 2010International audienceAims: We wish to separate and quantify the CO lumino...
This is the final version of the article. Available from American Astronomical Society and IOP Publi...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
23 pages, 22 PostScript figures. Accepted for publication in Astronomy & Astrophysics. Uses aa LaTeX...
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We have used archival far-ultraviolet spectra from observations made by HST/STIS and FUSE to determi...
International audienceContext: Most diffuse clouds are only known as kinematic features in absorptio...
5 pages, 1 PostScript figure. To be published in the proceedings of the Zermatt 2010 conference: ``C...
5 pages, 1 PostScript figure. To be published in the proceedings of the Zermatt 2010 conference: ``C...
Accepted to A&A 8 May 2010International audienceAims: We wish to separate and quantify the CO lumino...
Accepted to A&A 8 May 2010International audienceAims: We wish to separate and quantify the CO lumino...
This is the final version of the article. Available from American Astronomical Society and IOP Publi...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
Emission from carbon monoxide (CO) is ubiquitously used as a tracer of dense star-forming molecular ...
23 pages, 22 PostScript figures. Accepted for publication in Astronomy & Astrophysics. Uses aa LaTeX...
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We present a series of numerical simulations that explore how the ‘X-factor’, XCO – the conversion f...
We have used archival far-ultraviolet spectra from observations made by HST/STIS and FUSE to determi...
International audienceContext: Most diffuse clouds are only known as kinematic features in absorptio...