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The Spectrally Resolved Lyα Emission of Three Lyα-selected Field Galaxies at z ~ 2.4 from the HETDEX Pilot Survey
DOI: 10.1088/0004-637X/775/2/99 Bibcode: 2013ApJ...775...99C

Finkelstein, Steven L.; Kollmeier, Juna A.; Blanc, Guillermo A. +11 more

We present new results on the spectrally resolved Lyα emission of three Lyα-emitting field galaxies at z ~ 2.4 with high Lyα equivalent width (>100 Å) and Lyα luminosity (~1043 erg s-1). At 120 km s-1 (FWHM) spectral resolution, the prominent double-peaked Lyα profile straddles the systemic velocity, where the v…

2013 The Astrophysical Journal
eHST 44
RX J1301.9+2747: A Highly Variable Seyfert Galaxy with Extremely Soft X-Ray Emission
DOI: 10.1088/0004-637X/768/2/167 Bibcode: 2013ApJ...768..167S

Shu, Xinwen; Wang, Tinggui; Sun, Luming

In this paper we present a temporal and spectral analysis of X-ray data from XMM-Newton and Chandra observations of the ultrasoft and variable Seyfert galaxy RX J1301.9+2747. In both observations the source clearly displays two distinct states in the X-ray band: a long quiescent state and a short flare (or eruptive) state which differs in count ra…

2013 The Astrophysical Journal
XMM-Newton eHST 44
An X-Ray and Multiwavelength Survey of Highly Radio-loud Quasars at z > 4: Jet-linked Emission in the Brightest Radio Beacons of the Early Universe
DOI: 10.1088/0004-637X/763/2/109 Bibcode: 2013ApJ...763..109W

Brandt, W. N.; Schneider, Donald P.; Garmire, Gordon P. +3 more

We present a systematic study of the X-ray and multiwavelength properties of a sample of 17 highly radio-loud quasars (HRLQs) at z > 4 with sensitive X-ray coverage from new Chandra and archival Chandra, XMM-Newton, and Swift observations. Eight of the new and archival observations are reported in this work for the first time. New Chandra obser…

2013 The Astrophysical Journal
XMM-Newton 44
Late Spectral Evolution of the Ejecta and Reverse Shock in SN 1987A
DOI: 10.1088/0004-637X/768/1/88 Bibcode: 2013ApJ...768...88F

Fransson, Claes; Kirshner, Robert P.; Leibundgut, Bruno +10 more

We present observations with the Very Large Telescope and Hubble Space Telescope (HST) of the broad emission lines from the inner ejecta and reverse shock of SN 1987A from 1999 February until 2012 January (days 4381-9100 after explosion). We detect broad lines from Hα, Hβ, Mg I], Na I, [O I], [Ca II], and a feature at ~9220 Å. We identify the latt…

2013 The Astrophysical Journal
eHST 43
ALMA Continuum Observations of a 30 Myr Old Gaseous Debris Disk around HD 21997
DOI: 10.1088/2041-8205/777/2/L25 Bibcode: 2013ApJ...777L..25M

Apai, D.; Pascucci, I.; Ábrahám, P. +10 more

Circumstellar disks around stars older than 10 Myr are expected to be gas-poor. There are, however, two examples of old (30-40 Myr) debris-like disks containing a detectable amount of cold CO gas. Here we present Atacama Large Millimeter/Submillimeter Array (ALMA) and Herschel Space Observatory observations of one of these disks, around HD 21997, …

2013 The Astrophysical Journal
Herschel 43
The Magnetic Systems Triggering the M6.6 Class Solar Flare in NOAA Active Region 11158
DOI: 10.1088/0004-637X/773/2/128 Bibcode: 2013ApJ...773..128T

Toriumi, Shin; Kusano, Kanya; Inoue, Satoshi +3 more

We report a detailed event analysis of the M6.6 class flare in the active region (AR) NOAA 11158 on 2011 February 13. AR 11158, which consisted of two major emerging bipoles, showed prominent activity including one X- and several M-class flares. In order to investigate the magnetic structures related to the M6.6 event, particularly the formation p…

2013 The Astrophysical Journal
Hinode 43
A Super-solar Metallicity for the Progenitor of Kepler's Supernova
DOI: 10.1088/2041-8205/767/1/L10 Bibcode: 2013ApJ...767L..10P

Hughes, John P.; Lee, Jae-Joon; Mori, Koji +8 more

We have performed deep X-ray observations of the remnant of Kepler's supernova (SN 1604) as a Key Project of the Suzaku Observatory. Our main goal is to detect secondary Fe-peak elements in the supernova (SN) ejecta to gain insights into the Type Ia SN explosion mechanism and the nature of the progenitor. Here, we report our initial results. We ma…

2013 The Astrophysical Journal
Suzaku 43
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. IV. Recent Star Formation in NGC 602
DOI: 10.1088/0004-637X/775/1/68 Bibcode: 2013ApJ...775...68D

Panagia, Nino; Beccari, Giacomo; De Marchi, Guido

We have studied the young stellar populations in NGC 602, in the Small Magellanic Cloud, using a novel method that we have developed to combine Hubble Space Telescope photometry in the V, I, and Hα bands. We have identified about 300 pre-main-sequence (PMS) stars, all of which are still undergoing active mass accretion, and have determined their p…

2013 The Astrophysical Journal
eHST 43
Carbon Monoxide in the Cold Debris of Supernova 1987A
DOI: 10.1088/2041-8205/773/2/L34 Bibcode: 2013ApJ...773L..34K

Blommaert, J. A. D. L.; van Loon, J. Th.; Fransson, C. +27 more

We report spectroscopic and imaging observations of rotational transitions of cold CO and SiO in the ejecta of SN1987A, the first such emission detected in a supernova remnant. In addition to line luminosities for the CO J = 1-0, 2-1, 6-5, and 7-6 transitions, we present upper limits for all other transitions up to J = 13-12, collectively measured…

2013 The Astrophysical Journal
Herschel 43
Can the Differential Emission Measure Constrain the Timescale of Energy Deposition in the Corona?
DOI: 10.1088/0004-637X/774/1/31 Bibcode: 2013ApJ...774...31G

Parenti, S.; Auchère, F.; Klimchuk, J. A. +2 more

In this paper, the ability of the Hinode/EIS instrument to detect radiative signatures of coronal heating is investigated. Recent observational studies of active region cores suggest that both the low and high frequency heating mechanisms are consistent with observations. Distinguishing between these possibilities is important for identifying the …

2013 The Astrophysical Journal
Hinode 42