734 citations · 8.4k across the 62 of their papers we have counts for
62 papers
Down but not out: properties of the molecular gas in the stripped Virgo Cluster early-type galaxy NGC4526
Lisa M. Young, David S. Meier, Alison Crocker +2
We present ALMA data on the 3mm continuum emission, CO isotopologues (12CO, 13CO, C18O), and high-density molecular tracers (HCN, HCO+, HNC, HNCO, CS, CN, and CH3OH) in NGC4526. Th…
Binary Central Stars of Planetary Nebulae Identified With Kepler/K2
George H. Jacoby, Todd C. Hillwig, David Jones +6
We present the identification of 34 likely binary central stars (CSs) of planetary nebulae (PNe) from {\it Kepler/K2} data, seven of which show eclipses. Of these, 29 are new disco…
The Evolution of NGC 7465 as Revealed by its Molecular Gas Properties
Lisa M. Young, David S. Meier, Martin Bureau +3
We present ALMA observations of CO isotopologues and high-density molecular tracers (HCN, HCO+, CN, etc.) in NGC 7465, an unusually gas-rich early-type galaxy that acquired its col…
[CI](1-0) and [CI](2-1) in resolved local galaxies
Alison F. Crocker, Eric Pellegrini, J. -D. T. Smith +16
We present resolved [CI] line intensities of 18 nearby galaxies observed with the SPIRE FTS spectrometer on the Herschel Space Observatory. We use these data along with resolved CO…
Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH Sample
G. Aniano, B. T. Draine, L. K. Hunt +30
Dust and starlight are modeled for the KINGFISH project galaxies. With data from 3.6 micron to 500 micron, models are strongly constrained. For each pixel in each galaxy we estimat…
Using [CII] 158 micron Emission From Isolated ISM Phases as a Star-Formation Rate Indicator
Jessica Sutter, Daniel A. Dale, Kevin V. Croxall +17
The brightest observed emission line in many star-forming galaxies is the [CII] 158 micron line, making it detectable up to z~7. In order to better understand and quantify the [CII…