output
20022026
most citedStar Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

2k citations

Showing 2014 · astro-ph.SRShow all

10 papers · 2 filters

astro-ph.SR2014★ 29 cited

The JCMT Gould Belt Survey: Evidence for radiative heating in Serpens MWC 297 and its influence on local star formation

D. Rumble, J. Hatchell, R. A. Gutermuth +61

We present SCUBA-2 450micron and 850micron observations of the Serpens MWC 297 region, part of the JCMT Gould Belt Survey of nearby star-forming regions. Simulations suggest that r…

astro-ph.SR2014★ 78 cited

Sodium and Oxygen Abundances in the Open Cluster NGC 6791 from APOGEE H-Band Spectroscopy

Katia Cunha, Verne V. Smith, Jennifer A. Johnson +27

The open cluster NGC 6791 is among the oldest, most massive and metal-rich open clusters in the Galaxy. High-resolution -band spectra from the Apache Point Observatory Galactic…

astro-ph.SR2014★ 344 cited

The APOKASC Catalog: An Asteroseismic and Spectroscopic Joint Survey of Targets in the Kepler Fields

Marc H. Pinsonneault, Yvonne Elsworth, Courtney Epstein +42

We present the first APOKASC catalog of spectroscopic and asteroseismic properties of 1916 red giants observed in the Kepler fields. The spectroscopic parameters provided from the…

astro-ph.SR2014★ 109 cited

The Mass Budget of Planet Forming Discs: Isolating the Epoch of Planetesimal Formation

J. R. Najita, S. J. Kenyon

The high rate of planet detection among solar-type stars argues that planet formation is common. It is also generally assumed that planets form in protoplanetary discs like those o…

astro-ph.SR2014★ 38 cited

A Spitzer View of Mon OB1 East/NGC 2264

Valerie A. Rapson, Judith L. Pipher, Robert A. Gutermuth +4

We present Spitzer 3.6, 4.5, 5.8, 8.0, and 24 micron images of the Mon OB1 East giant molecular cloud, which contains the young star forming region NGC 2264, as well as more extend…

astro-ph.SR2014★ 12 cited

Kepler and the Long Period Variables

Erich Hartig, Jennifer Cash, Kenneth Hinkle +3

High precision Kepler photometry is used to explore the details of AGB light curves. Since AGB variability has a typical time scale on order of a year we discuss at length the remo…