output
19932026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2017 · astro-ph.GAShow all

189 papers · 2 filters

astro-ph.GA2017★ 3 cited

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud: III. Horizontal Branch Morphology

R. Wagner-Kaiser, Dougal Mackey, Ata Sarajedini +5

We leverage new high-quality data from Hubble Space Telescope program GO-14164 to explore the variation in horizontal branch morphology among globular clusters in the Large Magella…

astro-ph.GA2017★ 79 cited

Phosphorus-bearing molecules in the Galactic Center

V. M. Rivilla, I. Jiménez-Serra, S. Zeng +10

Phosphorus (P) is one of the essential elements for life due to its central role in biochemical processes. Recent searches have shown that P-bearing molecules (in particular PN and…

astro-ph.GA2017★ 3 cited

Experimental Indicators of Accretion Processes in Active Galactic Nuclei

A. Eckart, M. Valencia-S., B. Shahzamanian +19

Bright Active Galactic Nuclei are powered by accretion of mass onto the super massive black holes at the centers of the host galaxies. For fainter objects star formation may signif…

astro-ph.GA2017★ 69 cited

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

astro-ph.GA2017★ 8 cited

Gemini Spectra of Star Clusters in the Spiral Galaxy M101

Lesley A. Simanton-Coogan, Rupali Chandar, Bryan Miller +1

We present low resolution, visible light spectra of 41 star clusters in the spiral galaxy M101, taken with the Gemini/GMOS instrument. We measure Lick indices for each cluster and…

astro-ph.GA2017★ 88 cited

Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0

Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Ryan Brennan +37

The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (). We us…