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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2018, Volume 473, Issue 3, pp. 2899 - 2929
AbstractThe Central Molecular Zone (CMZ) of the Galactic Centre has to date only been fully mapped at mm wavelengths with single-dish telescopes, with... 
Molecular gases | Large scale structure of the universe | Photons | Iron | Velocity | Cosmic rays | Low energy | High energy astronomy | Wavelengths | Spectral resolution | Millimeter waves | Telescopes | Line spectra | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2018, Volume 473, Issue 3, pp. 2899 - 2929
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 08/2008, Volume 683, Issue 1, pp. L37 - L40
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 11/2019, Volume 885, Issue 1, p. 72
We have used the Goddard IRAM 2 Millimeter Observer (GISMO) with the 30 m IRAM telescope to carry out a 2 mm survey of the Galaxy’s central molecular zone.... 
Galaxies | Molecular clouds | Radio | Emissions | Dust emission | Point sources | Dust | H II regions | Wavelengths | Thermal emission | Interstellar chemistry | Filaments | Morphology | Interstellar medium | Interstellar matter | Interstellar gas
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 11/2019, Volume 885, Issue 1, p. 71
The central molecular zone, covering the inner ∼1° of the Galactic plane has been mapped at 2 mm using the Goddard-IRAM Superconducting 2-Millimeter Observer... 
Molecular clouds | Emission | Bolometers | Space telescopes | Emissions | Dust emission | Dust | Emissivity | Subtraction | Cosmic dust | Star formation | Filaments | Astrochemistry
Journal Article
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 2016, Volume 12, Issue 324, pp. 111 - 114
AbstractTwo modes of star formation are involved to explain the origin of young stars near Sgr A*. One is a disk-based mode, which explains the disk of stars... 
Galaxy: nucleus | stars: formation | ISM: clouds | Collapse | Star formation | Clouds | Molecular clouds | Galactic disk | Stars | Star clusters | Star & galaxy formation | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 05/2012, Volume 750, Issue 2, pp. L38 - 5
Journal Article
Astrophysical Journal, ISSN 0004-637X, 2017, Volume 845, Issue 1, p. 35
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 03/2009, Volume 694, Issue 1, pp. L16 - L20
OH(1720 MHz) masers are excellent signposts of interaction between supernova remnants (SNRs) and molecular clouds. Using the Green Bank Telescope and Very... 
Surveys | Shock waves | Supernova remnants | Masers | Radio lines: ISM | COMPLEX | MOLECULAR CLOUDS | surveys | masers | EXCITED MASER EMISSION | 1720 MHZ MASERS | radio lines: ISM | OH MASERS | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | GAS | B1757-24 | W28 | supernova remnants | shock waves | Physics - Astrophysics of Galaxies
Journal Article
Science, ISSN 0036-8075, 6/2002, Volume 296, Issue 5577, pp. 2350 - 2354
A supernova explosion, the final death throe of a massive star, creates an expanding bubble of hot gas that overruns up the surrounding medium. When a... 
Shock waves | Molecules | Supernova remnants | Reviews | Molecular gases | Molecular clouds | Masers | Molecular interactions | Photons | Hydroxyl masers | Magnetic fields | Supernovae | Influence | Evolution | Study and teaching | Cataclysmic variable stars | Research | Milky Way | Interstellar matter | Stars & galaxies | Astronomy
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 10/2006, Volume 650, Issue 1 I, pp. 203 - 211
We present the diffuse X-ray emission identified in Chandra observations of the young, massive Galactic star cluster Westerlund 1. After removing pointlike... 
Supernova remnants | Stars: winds, outflows | X-rays: stars | X-rays: ISM | POPULATION | stars : winds, outflows | X-rays : ISM | VORONOI TESSELLATIONS | X-rays : stars | REGION | SUPERNOVA-REMNANTS | ASTRONOMY & ASTROPHYSICS | RADIO-EMISSION | LARGE-MAGELLANIC-CLOUD | INITIAL MASS FUNCTION | supernova remnants | ARCHES CLUSTER | CHANDRA DETECTION | XMM-NEWTON
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2014, Volume 786, Issue 2
We have obtained improved spectra of key fundamental band lines of H3+, R(1,1)l, R(3,3)l, and R(2,2)l, and ro-vibrational transitions of CO on sightlines... 
Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 02/2006, Volume 637, Issue 2, pp. L101 - L104
A great deal of study has been conducted over the last 20 years on the origin of the magnetic activity in the Galactic center. One of the most popular... 
MHD | Turbulence | ISM: general | Galaxy: center | G359.54+0.18 | ISM : general | FLUX | turbulence | DISCOVERY | galaxy : center | CLOUDS | ASTRONOMY & ASTROPHYSICS | CENTER REGION | HIGH-RESOLUTION | DYNAMO THEORY | SPECTRUM | SIMULATIONS | SCATTERING
Journal Article
Astrophysical Journal, ISSN 0004-637X, 11/2011, Volume 741, Issue 2
The inner degrees of the Galactic center contain a large population of filamentary structures observed at radio frequencies. These so-called non-thermal radio... 
MAGNETIC FIELDS | TELESCOPES | ANTIPARTICLES | MATTER | ELECTRONS | ANNIHILATION | FERMIONS | ANTIMATTER | INTERACTIONS | ELEMENTARY PARTICLES | CROSS SECTIONS | LEPTONS | NONLUMINOUS MATTER | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ANTILEPTONS | PARTICLE INTERACTIONS | EMISSION SPECTRA | ELECTROMAGNETIC RADIATION | RADIATIONS | GALAXIES | EMISSION | SPECTRA | POSITRONS | VISIBLE RADIATION
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 2014, Volume 9, Issue 303, pp. 114 - 116
AbstractBecause of its large angular extent, the central molecular zone (CMZ) has to date only been mapped in the mm with single dish telescopes, with... 
radio lines: ISM | ISM: clouds | Galaxy: center | Stars & galaxies | Astronomy | Radio telescopes | Interferometry
Journal Article
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