X
Search Filters
Format Format
Subjects Subjects
Subjects Subjects
X
Sort by Item Count (A-Z)
Filter by Count
stars: formation (48) 48
physics - astrophysics of galaxies (47) 47
astronomy & astrophysics (44) 44
ism: clouds (44) 44
astrophysics - astrophysics of galaxies (41) 41
astrophysics (38) 38
galaxy astrophysics (27) 27
ism: molecules (26) 26
cosmology and extragalactic astrophysics (17) 17
ism: individual objects (17) 17
ism: kinematics and dynamics (17) 17
westerlund 2 (17) 17
radio lines: ism (13) 13
gas (12) 12
emission (11) 11
molecular clouds (11) 11
solar and stellar astrophysics (11) 11
star-formation (11) 11
clouds (8) 8
earth and planetary astrophysics (8) 8
evolution (8) 8
ism: individual (8) 8
turbulence (8) 8
astrophysics - solar and stellar astrophysics (7) 7
astrophysics, cosmology and astronomy (7) 7
isolating signatures (7) 7
h ii regions (6) 6
large-magellanic-cloud (6) 6
milky-way (6) 6
molecules (6) 6
-o-18 survey (5) 5
high energy astrophysical phenomena (5) 5
ism : clouds (5) 5
ism: structure (5) 5
magellanic clouds (5) 5
mass (5) 5
stars (5) 5
stars : formation (5) 5
young stellar objects (5) 5
carbon monoxide (4) 4
cores (4) 4
density (4) 4
h-ii regions (4) 4
massive stars (4) 4
sagittarius b2 (4) 4
star & galaxy formation (4) 4
2nd survey (3) 3
atomic-hydrogen (3) 3
catalog (3) 3
cluster formation (3) 3
co survey (3) 3
collision (3) 3
cosmology and extra-galactic astrophysics (3) 3
dark cloud (3) 3
dust (3) 3
filaments (3) 3
galactic plane (3) 3
galaxy (3) 3
gravitational-instability (3) 3
hydrogen (3) 3
initial conditions (3) 3
interstellar clouds (3) 3
ism : individual (3) 3
ism : molecules (3) 3
ism: atoms (3) 3
kinematics (3) 3
lmc (3) 3
molecular cloud (3) 3
molecular structure (3) 3
physics - solar and stellar astrophysics (3) 3
radio lines : ism (3) 3
stars: pre-main sequence (3) 3
super star cluster (3) 3
[phys.astr.co]physics [physics]/astrophysics [astro-ph]/cosmology and extra-galactic astrophysics [astro-ph.co] (2) 2
[phys.astr.ga]physics [physics]/astrophysics [astro-ph]/galactic astrophysics [astro-ph.ga] (2) 2
[phys.astr.he]physics [physics]/astrophysics [astro-ph]/high energy astrophysical phenomena [astro-ph.he] (2) 2
[phys.astr.im]physics [physics]/astrophysics [astro-ph]/instrumentation and methods for astrophysic [astro-ph.im] (2) 2
absorption (2) 2
alignment (2) 2
aperture synthesis (2) 2
apertures (2) 2
association (2) 2
astronomy (2) 2
balloons (2) 2
borders (2) 2
bubbling galactic disk (2) 2
chameleon-i (2) 2
chemistry (2) 2
circumstellar matter (2) 2
cloud-cloud collision (2) 2
clusters (2) 2
collisions (2) 2
comparative evaluations (2) 2
complex (2) 2
complex structure (2) 2
condensation (2) 2
continuum observations (2) 2
correlations (2) 2
dense cores (2) 2
disk (2) 2
more...
Language Language
Publication Date Publication Date
Click on a bar to filter by decade
Slide to change publication date range


The Astrophysical Journal, ISSN 1538-4357, 06/2019, Volume 878, Issue 2, p. 131
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 06/2017, Volume 69, Issue 3
Abstract Understanding massive cluster formation is one of the important issues of astronomy. By analyzing the H i data, we have identified that the two H i... 
stars: formation | Magellanic Clouds | ISM: individual (RMC 136) | H II regions
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 01/2019, Volume 871, Issue 1, p. 44
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2017, Volume 838, Issue 2
Comparison analyses between the gas emission data (H I 21 cm line and CO 2.6mm line) and the Planck/ IRAS dust emission data (optical depth at 353 GHz t353 and... 
ISM: atoms | ISM: molecules | ISM: individual objects (Perseus cloud) | PLANCK | CO-TO-H-2 CONVERSION FACTOR | ATOMIC GAS | H-2 | TRANSLUCENT CLOUDS | GALAXY | ASTRONOMY & ASTROPHYSICS | HIGH-RESOLUTION | INTERSTELLAR MOLECULAR-HYDROGEN | CONSTRAINTS | MILKY-WAY | Physics - Astrophysics of Galaxies
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 08/2019, Volume 71, Issue 4
Abstract The formation scenario of brown dwarfs is still unclear because observational studies to investigate its initial condition are quite limited. Our... 
ISM: individual objects (L1495, MC5-N) | SYSTEM | INITIAL CONDITIONS | MODEL | DEUTERIUM FRACTIONATION | (CO)-O-18 SURVEY | SCUBA-2 | stars: formation | DENSE CLOUD CORES | EVOLUTION | ASTRONOMY & ASTROPHYSICS | MOLECULAR GAS | 45-M | ISM: clouds | stars: low-mass | Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 04/2017, Volume 838, Issue 2, p. 132
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 08/2015, Volume 11, Issue S315, pp. 1 - 2
AbstractIt is crucially important to observe dense cores in order to investigate the initial condition of star formation since protostars are formed via... 
Molecules | Gases | Astrophysics | Star & galaxy formation | Kinematics | Collapse | Molecular structure | Star formation | Initial conditions | Continuums | Emission | Physical properties | Protostars
Journal Article
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, ISSN 0004-6264, 06/2017, Volume 69, Issue 3
Understanding massive cluster formation is one of the important issues of astronomy. By analyzing the HI data, we have identified that the two HI velocity... 
ISM: individual (RMC 136) | MOLECULAR CLOUDS | SUPER STAR CLUSTER | COLLISION | CO SURVEY | ISOLATING SIGNATURES | stars: formation | HYDROGEN | DUST | H II regions | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | GAS | Magellanic Clouds | LARGE-MAGELLANIC-CLOUD | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2018, Volume 860, Issue 1, p. 33
We carried out synthetic observations of interstellar atomic hydrogen at 21 cm wavelength by utilizing the magnetohydrodynamic numerical simulations of the... 
ISM: atoms | radio lines: ISM | ISM: clouds | APERTURE SYNTHESIS | MOLECULAR CLOUDS | NEUTRAL HYDROGEN | STAR-FORMATION | STRAY-RADIATION | 2ND SURVEY | EVOLUTION | ASTRONOMY & ASTROPHYSICS | ABSORPTION | LARGE-MAGELLANIC-CLOUD
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 835, Issue 2, p. 142
Understanding high-mass star formation is one of the top-priority issues in astrophysics. Recent observational studies have revealed that cloud-cloud... 
stars: formation | ISM: clouds | ISM: molecules | ISM: kinematics and dynamics | CORES | MOLECULAR CLOUDS | TELESCOPE | MYSTIX PROJECT | CLUSTER FORMATION | FORMING COMPLEX | ISOLATING SIGNATURES | YOUNG | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | TRIFID NEBULA | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/2019, Volume 871, Issue 1
The second most active site of high-mass star formation next to R136 in the Large Magellanic Cloud (LMC) is N44. We carried out a detailed analysis of H I at... 
stars: massive | H II regions | (galaxies:) Magellanic Clouds | ISM: atoms | galaxies: ISM | galaxies: star formation | MASSIVE STARS | APERTURE SYNTHESIS | MOLECULAR CLOUDS | DAY CHEMICAL-COMPOSITION | COLLISION | CO SURVEY | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | GAS | LARGE-MAGELLANIC-CLOUD | INTERSTELLAR COMPLEX
Journal Article
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, ISSN 0004-6264, 10/2018, Volume 70, Issue 5
We present Nobeyama 45 m telescope (CO)-O-18, (CO)-C-13, and (CO)-C-12(1-0) mapping observations towards an interstellar filament in the Taurus molecular... 
stars: formation | ASTRONOMY & ASTROPHYSICS | DENSE CORES | STAR-FORMATION | ISM: clouds | INTERSTELLAR-MEDIUM | TAURUS
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 02/2018, Volume 70, Issue 2, p. id.S52
Publications of the Astronomical Society of Japan, 2018 Formation mechanism of a supergiant H II region NGC 604 is discussed in terms of collision of H I... 
Physics - Astrophysics of Galaxies | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
No results were found for your search.

Cannot display more than 1000 results, please narrow the terms of your search.