Search Publications

Exploring the Possibility of O and Ne Contamination in Ulysses Observations of Interstellar Helium
DOI: 10.1088/0067-0049/220/2/31 Bibcode: 2015ApJS..220...31W

Wood, Brian E.; Müller, Hans-Reinhard; Möbius, Eberhard +4 more

We explore the possibility that interstellar O and Ne may be contributing to the particle signal from the GAS instrument on Ulysses, which is generally assumed to be entirely He. Motivating this study is the recognition that an interstellar temperature higher than any previously estimated from Ulysses data could potentially resolve a discrepancy b…

2015 The Astrophysical Journal Supplement Series
Ulysses 10
The Warm CO Gas along the UV-heated Outflow Cavity Walls: A Possible Interpretation for the Herschel/PACS CO Spectra of Embedded YSOs
DOI: 10.1088/0067-0049/217/2/30 Bibcode: 2015ApJS..217...30L

Lee, Jeong-Eun; Bergin, Edwin A.; Lee, Seokho

A fraction of the mid-J (J = 14-13 to J = 24-23) CO emission detected by the Herschel/Photodetector Array Camera and Spectrometer observations of embedded young stellar objects (YSOs) has been attributed to the UV-heated outflow cavity walls. We have applied our newly developed self-consistent models of photon-dominated-region (PDR) and non-local-…

2015 The Astrophysical Journal Supplement Series
Herschel 10
“Dust, Ice, and Gas In Time” (DIGIT) Herschel Observations of GSS30-IRS1 in Ophiuchus
DOI: 10.1088/0067-0049/217/1/6 Bibcode: 2015ApJS..217....6J

Lee, Jeong-Eun; Green, Joel D.; Je, Hyerin +2 more

As a part of the “Dust, Ice, and Gas In Time” (DIGIT) key program on Herschel, we observed GSS30-IRS1, a Class I protostar located in Ophiuchus (d = 120 pc), with Herschel/Photodetector Array Camera and Spectrometer. More than 70 lines were detected within a wavelength range from 50 to 200 µ m, including CO, H2O, OH, and two atomi…

2015 The Astrophysical Journal Supplement Series
Herschel 9
An Atlas of Bright Star Spectra in the Near-infrared from Cassini-VIMS
DOI: 10.1088/0067-0049/221/2/30 Bibcode: 2015ApJS..221...30S

Nicholson, Philip D.; Hedman, Matthew M.; Sloan, G. C. +2 more

We present the Cassini Atlas Of Stellar Spectra (CAOSS), comprised of near-infrared, low-resolution spectra of bright stars recovered from space-based observations by the Cassini spacecraft. The 65 stellar targets in the atlas are predominately M, K, and S giants. However, it also contains spectra of other bright nearby stars including carbon star…

2015 The Astrophysical Journal Supplement Series
Cassini 8
Star Cluster Disruption in the Starburst Galaxy Messier 82
DOI: 10.1088/0067-0049/216/1/6 Bibcode: 2015ApJS..216....6L

de Grijs, Richard; Li, Chengyuan; Li, Shuo +1 more

Using high-resolution, multiple-passband Hubble Space Telescope images spanning the entire optical/near-infrared wavelength range, we obtained a statistically complete U-band-selected sample of 846 extended star clusters across the disk of the nearby starburst galaxy M82. Based on a careful analysis of the clusters' spectral energy distributions, …

2015 The Astrophysical Journal Supplement Series
eHST 6
A CMB Gibbs Sampler for Localized Secondary Anisotropies
DOI: 10.1088/0067-0049/219/1/10 Bibcode: 2015ApJS..219...10B

Bull, Philip; Ferreira, Pedro G.; Wehus, Ingunn K. +4 more

In addition to primary fluctuations, cosmic microwave background (CMB) temperature maps contain a wealth of additional information in the form of secondary anisotropies. However, secondary effects that can be identified with individual objects, such as the thermal and kinetic Sunyaev-Zel’dovich (TSZ-KSZ) effects due to galaxy clusters, are difficu…

2015 The Astrophysical Journal Supplement Series
Planck 4