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Multi-wavelength Studies of Spectacular Ram-pressure Stripping of a Galaxy. II. Star Formation in the Tail
DOI: 10.1088/0004-637X/778/2/91 Bibcode: 2013ApJ...778...91Y

Makishima, Kazuo; Nakazawa, Kazuhiro; Gu, Liyi +5 more

With multiband photometric data in public archives, we detected four intracluster star-forming regions in the Virgo Cluster. Two of them were at a projected distance of 35 kpc from NGC 4388 and the other two were 66 kpc away. Our new spectroscopic observations revealed that their recessional velocities were comparable to the ram-pressure-stripped …

2013 The Astrophysical Journal
XMM-Newton 28
The Effects of Spatio-temporal Resolution on Deduced Spicule Properties
DOI: 10.1088/0004-637X/764/1/69 Bibcode: 2013ApJ...764...69P

De Pontieu, Bart; Carlsson, Mats; Pereira, Tiago M. D.

Spicules have been observed on the Sun for more than a century, typically in chromospheric lines such as Hα and Ca II H. Recent work has shown that so-called "type II" spicules may have a role in providing mass to the corona and the solar wind. In chromospheric filtergrams these spicules are not seen to fall back down, and they are shorter lived a…

2013 The Astrophysical Journal
Hinode 27
A Statistical Study of Coronal Active Events in the North Polar Region
DOI: 10.1088/0004-637X/775/1/22 Bibcode: 2013ApJ...775...22S

Shimojo, Masumi; Watanabe, Tetsuya; Sako, Nobuharu +1 more

In order to study the relationship between characteristics of polar coronal active events and the magnetic environment in which such events take place, we analyze 526 X-ray jets and 1256 transient brightenings in the polar regions and in regions around the equatorial limbs. We calculate the occurrence rates of these polar coronal active events as …

2013 The Astrophysical Journal
Hinode 27
Galaxy Halo Truncation and Giant Arc Surface Brightness Reconstruction in the Cluster MACSJ1206.2-0847
DOI: 10.1088/0004-637X/774/2/124 Bibcode: 2013ApJ...774..124E

Donahue, Megan; Broadhurst, Tom; Zheng, Wei +32 more

In this work, we analyze the mass distribution of MACSJ1206.2-0847, particularly focusing on the halo properties of its cluster members. The cluster appears relaxed in its X-ray emission, but has a significant amount of intracluster light that is not centrally concentrated, suggesting that galaxy-scale interactions are still ongoing despite the ov…

2013 The Astrophysical Journal
eHST 27
A Deep Search for Molecular Gas in Two Massive Lyman Break Galaxies at z = 3 and 4: Vanishing CO-emission Due to Low Metallicity?
DOI: 10.1088/2041-8205/776/2/L24 Bibcode: 2013ApJ...776L..24T

Daddi, E.; Elbaz, D.; Morrison, G. +14 more

We present deep IRAM Plateau de Bure Interferometer observations, searching for CO-emission toward two massive, non-lensed Lyman break galaxies at z = 3.216 and 4.058. With one low significance CO detection (3.5σ) and one sensitive upper limit, we find that the CO lines are gsim3-4 times weaker than expected based on the relation between IR and CO…

2013 The Astrophysical Journal
eHST 27
Uncovering the Deeply Embedded Active Galactic Nucleus Activity in the Nuclear Regions of the Interacting Galaxy Arp 299
DOI: 10.1088/2041-8205/779/1/L14 Bibcode: 2013ApJ...779L..14A

Alvarez, C.; Esquej, P.; Colina, L. +14 more

We present mid-infrared (MIR) 8-13 µm spectroscopy of the nuclear regions of the interacting galaxy Arp 299 (IC 694+NGC 3690) obtained with CanariCam (CC) on the 10.4 m Gran Telescopio Canarias (GTC). The high angular resolution (~0.''3-0.''6) of the data allows us to probe nuclear physical scales between 60 and 120 pc, which is a factor of …

2013 The Astrophysical Journal
eHST 27
X-Ray Grating Observations of Recurrent Nova T Pyxidis during the 2011 Outburst
DOI: 10.1088/0004-637X/779/1/22 Bibcode: 2013ApJ...779...22T

Ciroi, Stefano; Cracco, Valentina; Page, Kim L. +5 more

The recurrent nova T Pyx was observed with the X-ray gratings of Chandra and XMM-Newton, 210 and 235 days, respectively, after the discovery of the 2011 April 14 outburst. The X-ray spectra show prominent emission lines of C, N, and O, with broadening corresponding to an FWHM of ~2000-3000 km s-1, and line ratios consistent with high-de…

2013 The Astrophysical Journal
XMM-Newton 27
The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. II. M66 and M96 in the Leo I Group
DOI: 10.1088/0004-637X/773/1/13 Bibcode: 2013ApJ...773...13L

Lee, Myung Gyoon; Jang, In Sung

M66 and M96 in the Leo I Group are nearby spiral galaxies hosting Type Ia supernovae (SNe Ia). We estimate the distances to these galaxies from the luminosity of the tip of the red giant branch (TRGB). We obtain VI photometry of resolved stars in these galaxies from F555W and F814W images in the Hubble Space Telescope archive. From the luminosity …

2013 The Astrophysical Journal
eHST 27
Spectral Signatures of Penumbral Transients
DOI: 10.1088/0004-637X/779/2/143 Bibcode: 2013ApJ...779..143R

Katsukawa, Y.; Tritschler, A.; Reardon, K.

In this work we investigate the properties of penumbral transients observed in the upper photospheric and chromospheric region above a sunspot penumbra using two-dimensional spectroscopic observations of the Ca II 854.21 nm line with a 5 s cadence. In our 30 minutes of observations, we identify several penumbral-micro jets (PMJs) with cotemporal o…

2013 The Astrophysical Journal
Hinode 26
Discovery of Molecular Hydrogen in White Dwarf Atmospheres
DOI: 10.1088/2041-8205/766/2/L18 Bibcode: 2013ApJ...766L..18X

Koester, D.; Zuckerman, B.; Xu, S. +2 more

With the Cosmic Origins Spectrograph on board the Hubble Space Telescope, we have detected molecular hydrogen in the atmospheres of three white dwarfs with effective temperatures below 14,000 K, G29-38, GD 133, and GD 31. This discovery provides new independent constraints on the stellar temperature and surface gravity of white dwarfs.

2013 The Astrophysical Journal
eHST 26