搜索结果: 1-15 共查到“天文学 H2 x R”相关记录18条 . 查询时间(0.109 秒)
CO luminosity functions for far-infrared- and B-band-selected galaxies and the first estimate for Omega(H I+H2)
surveys molecules
2014/12/24
We derive a nonparametric CO luminosity function using an FIR- and an optical B-band-selected sample of the galaxies included in the FCRAO Extragalactic CO Survey. The FIR-selected sample is defined u...
When sticking influences H2 formation
ISM: dust, extinction – ISM: molecules – ISM: abundances
2011/10/20
Aims. Interstellar dust grains, because of their catalytic properties, are crucial to the formation of H2, the most abundant molecule in the Universe. The formation of molecular hydrogen strongly depe...
A survey for near-infrared H2 emission in Herbig Ae/Be stars: emission from the outer disks of HD 97048 and HD 100546
circumstellar matter, stars – pre-main-sequence, emission-line, protoplanetary disks
2011/9/30
We report on a sensitive search for H2 1-0 S(1), 1-0 S(0) and 2-1 S(1) ro-vibrational emission at 2.12, 2.22 and 2.25 micron in a sample of 15 Herbig Ae/Be stars employing CRIRES, the ESO-VLT near-inf...
The deeply obscured AGN of NGC4945 I. Spitzer-IRS maps of [Ne V], [Ne II], H2 0-0 S(1), S(2), and other tracers
Galaxies:active – Galaxies:nuclei – Galaxies:individual:NGC 4945 – ISM:lines and bands
2011/9/27
The nearly edge-on galaxy NGC4945 is one of the closest galaxies where an AGN and starburst coexist, and is one of the brightest sources at 100 keV. Near and mid-infrared spectroscopy have shown very ...
How Universal is the SFR - H2 Relation?
Cosmology and Extragalactic Astrophysics (astro-ph.CO) Galaxy Astrophysics (astro-ph.GA)
2010/12/27
It is a well established empirical fact that the surface density of the star formation rate, Sigma_SFR, strongly correlates with the surface density of molecular hydrogen, Sigma_H2, at least when aver...
Spitzer Mapping of PAHs and H2 in Photodissociation Regions
Galaxy Astrophysics (astro-ph.GA)
2010/12/22
The mid-infrared (MIR) spectra of dense photodissociation regions (PDRs) are typically dominated by emission from polycyclic aromatic hydrocarbons (PAHs) and the lowest pure rotational states of molec...
H2 velocity structure in the molecular outflow dr 21
H2 velocity structure molecular outflow dr 21
2009/7/9
H2 velocity structure in the molecular outflow dr 21。
The Use of KS Band Photometric Excesses to Investigate H2 Emission in Planetary Nebulae
KS Band Photometric Planetary Nebulae H2 Emission
2009/6/30
The Use of KS Band Photometric Excesses to Investigate H2 Emission in Planetary Nebulae。
The N(H2)/I(CO) Conversion Factor:A Treatment that Includes Radiative Transfer
Conversion Factor N(H2)/I(CO) Radiative Transfer
2009/6/30
The N(H2)/I(CO) Conversion Factor:A Treatment that Includes Radiative Transfer。
The Formation of H2 in Variable Herbig-Haro Jets。
The Formation of H2 in Variable Herbig-Haro Jets。
H2 Velocity Structure in HH 211。
Spatial distribution of H2 Fluorescence in the Inner 2x2 around T Tau
H2 Fluorescence Inner 2x2 T Tau
2009/6/15
Spatial distribution of H2 Fluorescence in the Inner 2x2 around T Tau。
H2 observations of outflows from young stars。