The herschel view_of_massive_star_formation_in_dense_and_cold_filament_w48
Dust production and_particle_acceleration_in_supernova_1987_a_revealed_with_alma
Aa20797 12
A herschel and_apex_census_of_the_reddest_sources_in_orion_searching_for_the_youngest_protostars
Astronauts and Robots 2015: Jonas Zmuidzinas, JPL
Stephan Ott (Herschel Science Centre, ESTEC) on behalf of the Herschel Science Ground Segment Consortium .
VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.
WP6200 : Padova Scientific Activities
ESA/NASA/Hubble Astronomy is a dynamic and ever-changing science, where new discoveries are regularly made. Many thousands of astronomers around the world.
Bill Reach 2009 May 14 Greater IPAC Technology Symposium.
Calculation of Highly Accurate Rovibrational Spectra for Molecules Containing a Large-Amplitude Motion: Ammonia Xinchuan Huang, David W. Schwenke, Timothy.
Astronomy highlights during IYA2009
![VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.](https://static.fdocuments.in/doc/330x215/56649edb5503460f94bea5fd/vngs-science-highlight-pdr-models-of-m51-ciioi63-ciioi63f-tir.jpg)
