X
Search Filters
Format Format
Subjects Subjects
Subjects Subjects
X
Sort by Item Count (A-Z)
Filter by Count
astronomy & astrophysics (70) 70
158 mu-m (40) 40
astrophysics (31) 31
photodissociation regions (29) 29
galaxies: ism (27) 27
interstellar-medium (26) 26
astrophysics - astrophysics of galaxies (25) 25
physics - astrophysics of galaxies (22) 22
cosmology and extragalactic astrophysics (21) 21
galaxy astrophysics (21) 21
158 micron (20) 20
galaxies (19) 19
galaxies: high-redshift (17) 17
active galactic nuclei (15) 15
high energy astrophysical phenomena (14) 14
physical conditions (14) 14
c-ii line (13) 13
emission (13) 13
star-formation rate (13) 13
astrophysics - cosmology and nongalactic astrophysics (12) 12
molecular gas (12) 12
astronomy (11) 11
physics (11) 11
star-formation (11) 11
earth and planetary astrophysics (10) 10
galaxies: star formation (10) 10
infrared: galaxies (10) 10
luminosity (10) 10
polycyclic aromatic-hydrocarbons (10) 10
star formation (10) 10
ultraluminous infrared galaxies (10) 10
astrophysics, cosmology and astronomy (9) 9
carbon (9) 9
cosmology: observations (9) 9
dust (9) 9
galaxies: starburst (9) 9
red shift (9) 9
solar and stellar astrophysics (9) 9
c-ii (8) 8
far-infrared spectroscopy (8) 8
forming galaxies (8) 8
galaxies: evolution (8) 8
ism: lines and bands (8) 8
space-observatory measurements (8) 8
158 micron line (7) 7
gas (7) 7
h-ii regions (7) 7
high-redshift (7) 7
high-redshift galaxies (7) 7
host galaxies (7) 7
infrared: ism (7) 7
ism: clouds (7) 7
neutral atomic phases (7) 7
physics - cosmology and nongalactic astrophysics (7) 7
star-forming galaxies (7) 7
stars (7) 7
[phys.astr]physics [physics]/astrophysics [astro-ph] (6) 6
cii emission (6) 6
dust, extinction (6) 6
galaxies: individual (6) 6
large-magellanic-cloud (6) 6
line emission (6) 6
molecular clouds (6) 6
quasars (6) 6
spectral energy-distribution (6) 6
density (5) 5
excitation (5) 5
galaxies : ism (5) 5
galaxies: active (5) 5
galaxies: formation (5) 5
infrared (5) 5
ism: structure (5) 5
milky-way (5) 5
physics and astronomy (5) 5
spectral energy-distributions (5) 5
star evolution (5) 5
submillimeter galaxies (5) 5
astrochemistry (4) 4
clouds (4) 4
correlations (4) 4
evolution (4) 4
giant molecular clouds (4) 4
infrared, ism, lines and bands (4) 4
infrared: ism: lines and bands (4) 4
ism: atoms (4) 4
ism: general (4) 4
ism: molecules (4) 4
line (4) 4
magellanic clouds (4) 4
mathematical models (4) 4
mu-m (4) 4
radiative transfer (4) 4
submillimeter (4) 4
submillimeter: ism (4) 4
submillimetre: galaxies (4) 4
techniques: spectroscopic (4) 4
[ phys.astr ] physics [physics]/astrophysics [astro-ph] (3) 3
[phys.astr.co]physics [physics]/astrophysics [astro-ph]/cosmology and extra-galactic astrophysics [astro-ph.co] (3) 3
[phys.astr.ga]physics [physics]/astrophysics [astro-ph]/galactic astrophysics [astro-ph.ga] (3) 3
[phys.astr.he]physics [physics]/astrophysics [astro-ph]/high energy astrophysical phenomena [astro-ph.he] (3) 3
more...
Language Language
Publication Date Publication Date
Click on a bar to filter by decade
Slide to change publication date range


ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 09/2005, Volume 440, Issue 2, pp. L51 - L54
We report the detection of the P-2(3/2) -> P-2(1/2) fine-structure line of C+ at 157.74 mu m in SDSS J114816.64+525150.3 ( hereafter J1148+5251), the most... 
galaxies : high redshift | PHYSICAL CONDITIONS | quasars : individual : J114816.64+525150.3 | ISM : abundances | INTERSTELLAR-MEDIUM | 158 MICRON C | submillimeter | LINE DEFICIT | Z=6.42 | galaxies : ISM | DUST | QUASARS | II EMISSION | ASTRONOMY & ASTROPHYSICS | infrared : galaxies | HOST GALAXY | ULTRALUMINOUS INFRARED GALAXIES
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 06/2017, Volume 842, Issue 1
With its relatively low ionization potential, C+ can be found throughout the interstellar medium (ISM) and provides one of the main cooling channels of the ISM... 
NEARBY GALAXIES | WARM IONIZED MEDIUM | NEUTRAL ATOMIC PHASES | PHYSICAL CONDITIONS | galaxies: ISM | STAR-FORMATION RATE | HIGH GALACTIC LATITUDE | ASTRONOMY & ASTROPHYSICS | C-II LINE | FAR-INFRARED SPECTROSCOPY | MICRON LINE | 158 MU-M
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 03/2015, Volume 801, Issue 2
We present ALMA observations of two moderate-luminosity quasars at redshift 6. These quasars, from the Canada France High-z Quasar Survey (CFHQS), have black... 
quasars: general | galaxies: evolution | LUMINOSITY FUNCTION | galaxies: high-redshift | 158 MU-M | DUST | QUASARS | EVOLUTION | ACTIVE GALACTIC NUCLEI | ASTRONOMY & ASTROPHYSICS | FORMING GALAXY | MOLECULAR GAS | cosmology: observations | C II LINE | EMISSION
Journal Article
Publications of the Astronomical Society of the Pacific, ISSN 0004-6280, 12/2011, Volume 123, Issue 910, pp. 1347 - 1369
The KINGFISH project (Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel) is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc)... 
Online material: extended figure | RADIAL-DISTRIBUTION | MAGELLANIC-CLOUD | COLD DUST | STAR-FORMATION RATES | FORMING GALAXIES | ASTRONOMY & ASTROPHYSICS | H-ALPHA KINEMATICS | SPECTRAL ENERGY-DISTRIBUTION | 158 MU-M | HII-REGIONS | FORMATION HISTORIES | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2015, Volume 807, Issue 2, pp. 1 - 9
Journal Article
The Astrophysical Journal: an international review of astronomy and astronomical physics, ISSN 0004-637X, 01/2017, Volume 834, Issue 1, p. 5
Journal Article
Astrophysical Journal, ISSN 0004-637X, 11/2015, Volume 813, Issue 1, p. 36
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 2, p. 168
Using the Very Large Array and ALMA, we have obtained CO(2-1), [C II], and [N II] line emission and multiple dust continuum measurements in a sample of... 
PHYSICAL CONDITIONS | galaxies: star formation | MU-M | STARBURST GALAXY | galaxies: high-redshift | galaxies: formation | radio lines: galaxies | SUBMILLIMETER GALAXIES | FORMING GALAXIES | PHOTODISSOCIATION REGIONS | galaxies: ISM | HIGH-REDSHIFT | ASTRONOMY & ASTROPHYSICS | C-II LINE | MOLECULAR GAS | cosmology: observations | 158 MICRON
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 10/2016, Volume 462, Issue 1, pp. L6 - L10
The far-infrared fine-structure line [C II] at 1900.5 GHz is known to be one of the brightest cooling lines in local galaxies, and therefore it has been... 
LOW DUST | galaxies: evolution | HOST GALAXIES | LYMAN BREAK GALAXIES | galaxies: high-redshift | 158 MU-M | HUBBLE | galaxies: formation | galaxies: ISM | HIGH-REDSHIFT | ASTRONOMY & ASTROPHYSICS | LINE | GAS | LY-ALPHA EMISSION | SPECTROSCOPIC CONFIRMATION | submillimetre: galaxies | Physics | Astrophysics
Journal Article
Publications of the Astronomical Society of the Pacific, ISSN 0004-6280, 06/2013, Volume 125, Issue 928, pp. 600 - 635
The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies using 230 hr of far-infrared (FIR) and submillimetre (submm) photometric and... 
Article | ASTROPHYSICAL DUST EMISSION | AROMATIC-HYDROCARBON EMISSION | STAR-FORMING GALAXIES | HUBBLE-SPACE-TELESCOPE | LOW-METALLICITY ENVIRONMENTS | ASTRONOMY & ASTROPHYSICS | H-II REGIONS | BLUE COMPACT GALAXIES | SPECTRAL ENERGY-DISTRIBUTION | NEUTRAL HYDROGEN OBSERVATIONS | 158 MU-M | Sciences of the Universe | Astrophysics
Journal Article