Results 271 to 280 of about 71,444 (299)
Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P +21 more
europepmc +1 more source
Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Submillimeter Dust Continuum Emission as a Probe of Protostellar Evolution
1996The strength and spatial distribution of the (sub)millimeter continuum emission from young stellar objects (YSOs) are powerful diagnostics of the progressive decrease and condensation of circumstellar mass during protostellar evolution. In particular, the ratio of submm to bolometric luminosity may be used as a practical evolutionary indicator for ...
Philippe André, Sylvain Bontemps
openaire +1 more source
Millimeter Dust Continuum Emission as a Tracer of Molecular Gas in Galaxies
2008Molecular gas in galaxies is the primary fuel of star formation but the exact amount of molecular gas remains unknown since H_2 is not observed directly in cold interstellar regions. CO observations have been so far the best way to trace molecular gas in external galaxies, but in low metallicity environments the gas mass deduced could be largely ...
Bot, Caroline +3 more
openaire +2 more sources
The Mass-Loss History of Carbon Stars Probed by Co Line and Dust Continuum Emission
2003An extensive modelling of CO line emission from the circumstellar envelopes around a number of carbon stars is performed. By combining radio observations and infrared observations obtained by ISO the circumstellar envelope characteristics are probed over a large radial range.
Fredrik Larsen Schöier +2 more
openaire +1 more source
Journal of Experimental and Theoretical Physics, 2008
The continuum approximation is used to analyze the effect of electron emission from the surface of a spherical dust grain immersed in a plasma on the grain charge by assuming negligible ionization and recombination in the disturbed plasma region around the grain.
D'yachkov, L., Khrapak, A., Khrapak, S.
openaire +2 more sources
The continuum approximation is used to analyze the effect of electron emission from the surface of a spherical dust grain immersed in a plasma on the grain charge by assuming negligible ionization and recombination in the disturbed plasma region around the grain.
D'yachkov, L., Khrapak, A., Khrapak, S.
openaire +2 more sources
Search for massive protostar candidates in the southern hemisphere. II. Dust continuum emission
2006In an ongoing effort to identify and study high-mass protostellar candidates we have observed in various tracers a sample of 235 sources selected from the IRAS Point Source Catalog, mostly with δ < -30 degr, with the SEST antenna at millimeter wavelengths.
Beltr +7 more
openaire +1 more source
Appendices to "ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion"
Appendices A through H to the A&A publication "ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion" by T. Danilovich, N. Samaratunge, Y. Mori, A. M. S. Richards, A. Baudry, S. Etoka, M. Montargès, P. Kervella, I. McDonald, C. A. Gottlieb, A. Wallace, D. J. Price, L. Decin, J. Bolte, T. Ceulemans, F. De Ceuster, A.openaire +1 more source
2008
The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution, 14-16 November, 2005, Pasadena, California ...
Leeuw, L. L. +5 more
openaire +1 more source
The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution, 14-16 November, 2005, Pasadena, California ...
Leeuw, L. L. +5 more
openaire +1 more source

