Search Publications

Hubble Space Telescope Emission Line Galaxies at z ~ 2: The Lyα Escape Fraction
DOI: 10.1088/0004-637X/796/1/64 Bibcode: 2014ApJ...796...64C

Schneider, Donald P.; Blanc, Guillermo A.; Gronwall, Caryl +8 more

We compare the Hβ line strengths of 1.90 < z < 2.35 star-forming galaxies observed with the near-IR grism of the Hubble Space Telescope with ground-based measurements of Lyα from the HETDEX Pilot Survey and narrow-band imaging. By examining the line ratios of 73 galaxies, we show that most star-forming systems at this epoch have a Lyα escape…

2014 The Astrophysical Journal
eHST 30
A Search for Companions to Brown Dwarfs in the Taurus and Chamaeleon Star-Forming Regions
DOI: 10.1088/0004-637X/788/1/40 Bibcode: 2014ApJ...788...40T

Todorov, K. O.; Luhman, K. L.; Konopacky, Q. M. +5 more

We have used WFPC2 on board the Hubble Space Telescope to obtain images of 47 members of the Taurus and Chamaeleon I star-forming regions that have spectral types of M6-L0 (M ~ 0.01-0.1 M ). An additional late-type member of Taurus, FU Tau (M7.25+M9.25), was also observed with adaptive optics at Keck Observatory. In these images, we ha…

2014 The Astrophysical Journal
eHST 30
Observational Studies on the Near-infrared Unidentified Emission Bands in Galactic H II Regions
DOI: 10.1088/0004-637X/784/1/53 Bibcode: 2014ApJ...784...53M

Onaka, Takashi; Sakon, Itsuki; Shimonishi, Takashi +4 more

Using a large collection of near-infrared spectra (2.5-5.4 µm) of Galactic H II regions and H II region-like objects, we perform a systematic investigation of astronomical polycyclic aromatic hydrocarbon (PAH) features. Thirty-six objects were observed using the infrared camera on board the AKARI satellite as a part of a director's time prog…

2014 The Astrophysical Journal
AKARI 30
The Spatially Resolved Bipolar Nebula of Sakurai's Object
DOI: 10.1088/0004-637X/785/2/146 Bibcode: 2014ApJ...785..146H

Hinkle, Kenneth H.; Joyce, Richard R.

Sakurai's object (V4334 Sgr), the final flash object discovered in the mid-1990s, underwent rapid cooling during the first decade of the 21st century becoming as faint as K ~ 25. This stage of evolution has ceased. Between observations in 2010 September and 2013 April V4334 Sgr brightened >2 mag to K = 14.2 and the effective temperature increas…

2014 The Astrophysical Journal
eHST 30
Not-so-simple Stellar Populations in the Intermediate-age Large Magellanic Cloud Star Clusters NGC 1831 and NGC 1868
DOI: 10.1088/0004-637X/784/2/157 Bibcode: 2014ApJ...784..157L

Deng, Licai; de Grijs, Richard; Li, Chengyuan

Using a combination of high-resolution Hubble Space Telescope/Wide-Field and Planetary Camera-2 observations, we explore the physical properties of the stellar populations in two intermediate-age star clusters, NGC 1831 and NGC 1868, in the Large Magellanic Cloud based on their color-magnitude diagrams. We show that both clusters exhibit extended …

2014 The Astrophysical Journal
eHST 30
High-resolution Submillimeter and Near-infrared Studies of the Transition Disk around Sz 91
DOI: 10.1088/0004-637X/783/2/90 Bibcode: 2014ApJ...783...90T

Henning, Thomas; Terada, Hiroshi; Usuda, Tomonori +55 more

To reveal the structures of a transition disk around a young stellar object in Lupus, Sz 91 , we have performed aperture synthesis 345 GHz continuum and CO(3-2) observations with the Submillimeter Array (~1''-3'' resolution) and high-resolution imaging of polarized intensity at the Ks -band using the HiCIAO instrument on the Subaru Tele…

2014 The Astrophysical Journal
Herschel 30
X-Ray and γ-Ray Studies of the Millisecond Pulsar and Possible X-Ray Binary/Radio Pulsar Transition Object PSR J1723-2837
DOI: 10.1088/0004-637X/781/1/6 Bibcode: 2014ApJ...781....6B

Esposito, Paolo; Bogdanov, Slavko; McLaughlin, Maura A. +3 more

We present X-ray observations of the "redback" eclipsing radio millisecond pulsar (MSP) and candidate radio pulsar/X-ray binary transition object PSR J1723-2837. The X-ray emission from the system is predominantly non-thermal and exhibits pronounced variability as a function of orbital phase, with a factor of ~2 reduction in brightness around supe…

2014 The Astrophysical Journal
XMM-Newton 30
The Comparison of Physical Properties Derived from Gas and Dust in a Massive Star-forming Region
DOI: 10.1088/0004-637X/786/2/116 Bibcode: 2014ApJ...786..116B

Ginsburg, Adam; Battersby, Cara; Bally, John +3 more

We explore the relationship between gas and dust in a massive star-forming region by comparing the physical properties derived from each. We compare the temperatures and column densities in a massive star-forming Infrared Dark Cloud (G32.02+0.05), which shows a range of evolutionary states, from quiescent to active. The gas properties were derived…

2014 The Astrophysical Journal
Herschel 29
Herschel Evidence for Disk Flattening or Gas Depletion in Transitional Disks
DOI: 10.1088/0004-637X/787/2/153 Bibcode: 2014ApJ...787..153K

Dent, W. R. F.; Woitke, P.; Kamp, I. +6 more

Transitional disks are protoplanetary disks characterized by reduced near- and mid-infrared emission, with respect to full disks. This characteristic spectral energy distribution indicates the presence of an optically thin inner cavity within the dust disk believed to mark the disappearance of the primordial massive disk. We present new Herschel S…

2014 The Astrophysical Journal
Herschel 29
The Tip of the Red Giant Branch Distance to the Perfect Spiral Galaxy M74 Hosting Three Core-collapse Supernovae
DOI: 10.1088/0004-637X/792/1/52 Bibcode: 2014ApJ...792...52J

Lee, Myung Gyoon; Jang, In Sung

M74 (NGC 628) is a famous face-on spiral galaxy, hosting three core-collapse supernovae (SNe): SN Ic 2002ap, SN II-P 2003gd, and SN II-P 2013ej. However, its distance is not well known. We present a distance estimation for this galaxy based on the Tip of the Red Giant Branch (TRGB) method. We obtain photometry of the resolved stars in the arm-free…

2014 The Astrophysical Journal
eHST 29