2.5k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Ames Research CenterUS866 papers
- Center for Astrophysics Harvard & SmithsonianUS447 papers
- California Institute of TechnologyUS416 papers
- Centre National de la Recherche ScientifiqueFR394 papers
- University of California, BerkeleyUS388 papers
- Space Telescope Science InstituteUS351 papers
- Massachusetts Institute of TechnologyUS319 papers
- Goddard Space Flight CenterUS295 papers
- Princeton UniversityUS258 papers
- Jet Propulsion LaboratoryUS249 papers
- University of California, Santa CruzUS229 papers
- University of ArizonaUS213 papers
17 papers · 2 filters
Families and Clusters of Diffuse Interstellar Bands: a Data-Driven Correlation Analysis
Haoyu Fan, Madison Schwartz, Amin Farhang +9
More than 500 diffuse interstellar bands (DIBs) have been observed in astronomical spectra, and their signatures and correlations in different environments have been studied over t…
C diffuse interstellar band correlations and environmental variations
Leander Schlarmann, Bernard Foing, Jan Cami +1
The Diffuse Interstellar Bands (DIBs) are absorption features seen in the spectra of astronomical objects, that arise in the interstellar medium. Today more than 500 DIBs have been…
Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC+ and comparing with simulation
Pak Shing Li, Enrique Lopez-Rodriguez, Hamza Ajeddig +4
Optical and infrared polarization mapping and recent Planck observations of the filamentary cloud L1495 in Taurus show that the large-scale magnetic field is approximately perpendi…
Characterizing Spatial Variations of PAH Emission in the Reflection Nebula NGC 1333
C. Knight, E. Peeters, M. Wolfire +1
Infrared emission features at 3.3, 6.2, 7.7, 8.6, and 11.2 m, attributed to polycyclic aromatic hydrocarbons, show variations in relative intensity, shape, and peak position. Th…
CO emission as an effective measure of gas masses of protoplanetary disks
Maxime Ruaud, Uma Gorti, David Hollenbach
Many astrochemical models of observed CO isotopologue line emission, earlier considered a good proxy measure of H and hence disk gas mass, favor large deviations in the carbon…
The MURALES survey. V. Jet-induced star formation in 3C 277.3 (Coma A)
A. Capetti, B. Balmaverde, C. Tadhunter +13
We present observations obtained with the VLT/MUSE optical integral field spectrograph of the radio source 3C277.3, located at a redshift of 0.085 and associated with the galaxy Co…
The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
P. Scicluna, F. Kemper, I. McDonald +89
The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of 850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO (21) and…
Characterizing the PAH Emission in the Orion Bar
C. Knight, E. Peeters, A. G. G. M. Tielens +1
We present 5--14~m spectra at two different positions across the Orion Bar photodissociation region (PDR) obtained with the Infrared Spectrograph onboard the Spitzer Space Teles…
A Spectroscopic Study of Supernova Remnants with the Infrared Space Observatory
Matthew J. Millard, Aravind P. Ravi, Jeonghee Rho +1
We present far-infrared (FIR) spectroscopy of supernova remnants (SNRs) based on the archival data of the Infrared Space Observatory () taken with the Long Wavelength Spectrom…
The MURALES survey. IV. Searching for nuclear outflows in 3C radio galaxies at z < 0.3 with MUSE observations
Giovanna Speranza, Barbara Balmaverde, Alessandro Capetti +13
We analyze VLT/MUSE observations of 37 radio galaxies from the Third Cambridge catalogue (3C) with redshift 0.3 searching for nuclear outflows of ionized gas. These observations…
Tracing PAH Size in Prominent Nearby Mid-Infrared Environments
C. Knight, E. Peeters, D. J. Stock +2
We present observations from the First Light Infrared TEst CAMera (FLITECAM) on board the Stratospheric Observatory for Infrared Astronomy (SOFIA), the Spitzer Infrared Array Camer…
Shocked Molecular Hydrogen and Broad CO lines from the Interacting Supernova Remnant HB 3
J. Rho, T. H. Jarrett, L. N. Tram +6
We present the detections of shocked molecular hydrogen (H2) gas in near- and mid-infrared and broad CO in millimeter from the mixed-morphology supernova remnant (SNR) HB~3 (G132.7…
Raining in MKW 3s: a Chandra-MUSE analysis of X-ray cold filaments around 3CR 318.1
A. Jimenez-Gallardo, F. Massaro, B. Balmaverde +23
We present the analysis of X-ray and optical observations of gas filaments observed in the radio source 3CR 318.1, associated with NGC 5920, the Brightest Cluster Galaxy (BCG) of M…
H2 ro-vibrational excitation in protoplanetary disks and its effects on the chemistry
Maxime Ruaud
The effect of H ro-vibrational excitation on the chemistry of protoplanetary disks is studied using a framework that solves for the disk physical and chemical structure and inc…
Sagittarius B1 -- A Patchwork of H II Regions and PhotoDissociation Regions
Janet P. Simpson, Sean W. J. Colgan, Angela S. Cotera +2
Sgr B1 is a luminous H II region in the Galactic Center immediately next to the massive star-forming giant molecular cloud Sgr B2 and apparently connected to it from their similar…
Hunting for Planetary Nebulae toward the Galactic Center
Jihye Hong, Janet P. Simpson, Deokkeun An +2
We present near-infrared (IR) spectra of two planetary nebula (PN) candidates in close lines of sight toward the Galactic center (GC) using the Gemini Near-Infrared Spectrograph (G…
The Galactic Faraday rotation sky 2020
Sebastian Hutschenreuter, Craig S. Anderson, Sarah Betti +34
This work gives an update to existing reconstructions of the Galactic Faraday rotation sky by processing almost all Faraday rotation data sets available at the end of the year 2020…