output
19962026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations

Showing 2015 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2015★ 84 cited

High-resolution IR absorption spectroscopy of polycyclic aromatic hydrocarbons: the realm of anharmonicity

Elena Maltseva, Annemieke Petrignani, Alessandra Candian +6

We report on an experimental and theoretical investigation of the importance of anharmonicity in the 3 micron CH stretching region of Polycyclic Aromatic Hydrocarbon (PAH) molecule…

astro-ph.GA2015★ 153 cited

Measuring the vertical age structure of the Galactic disc using asteroseismology and SAGA

L. Casagrande, V. Silva Aguirre, K. J. Schlesinger +10

The existence of a vertical age gradient in the Milky Way disc has been indirectly known for long. Here, we measure it directly for the first time with seismic ages, using red gian…

astro-ph.GA2015★ 14 cited

Mid-infrared spectroscopy of the Andromeda galaxy

D. Hemachandra, P. Barmby, E. Peeters +6

We present Spitzer/Infrared Spectrograph (IRS) 5-21 micron spectroscopic maps towards 12 regions in the Andromeda galaxy (M31). These regions include the nucleus, bulge, an active…

astro-ph.GA2015★ 269 cited

Stars, Gas, and Dark Matter in the Solar Neighborhood

Christopher F. McKee, Antonio Parravano, David J. Hollenbach

The surface density and vertical distribution of stars, stellar remnants, and gas in the solar vicinity form important ingredients for understanding the star formation history of t…

astro-ph.GA2015★ 92 cited

Excitation Mechanisms for HCN (1-0) and HCO+ (1-0) in Galaxies from the Great Observatories All-sky LIRG Survey

G. C. Privon, R. Herrero-Illana, A. S. Evans +18

We present new IRAM 30m spectroscopic observations of the GHz band, including emission from the CCH (n=1-0) multiplet, HCN (1-0), HCO+ (1-0), and HNC (1-0), for a sample o…

astro-ph.GA2015★ 10 cited

Detection of Extremely Broad Water Emission from the molecular cloud interacting Supernova Remnant G349.7+0.2

J. Rho, J. W. Hewitt, A. Boogert +2

We performed Herschel HIFI, PACS and SPIRE observations towards the molecular cloud interacting supernova remnant G349.7+0.2. An extremely broad emission line was detected at 557 G…