Search Publications

Baryonic Tully-Fisher relation for extremely low mass Galaxies
DOI: 10.1111/j.1365-2966.2008.13010.x Bibcode: 2008MNRAS.386..138B

Sharina, M. E.; Begum, Ayesha; Chengalur, Jayaram N. +1 more

We study Tully-Fisher (TF) relations for a sample that combines extremely faint (MB < -14) galaxies along with bright (i.e. ~L*) galaxies. Accurate (~10 per cent) distances, I-band photometry and B - V colours are known for the majority of the galaxies in our sample. The faint galaxies are drawn from the Faint Irregular Ga…

2008 Monthly Notices of the Royal Astronomical Society
eHST 77
Persistent Horizontal Flows and Magnetic Support of Vertical Threads in a Quiescent Prominence
DOI: 10.1086/595785 Bibcode: 2008ApJ...689L..73C

Chae, Jongchul; Choe, G. S.; Lim, Eun-Kyung +2 more

There has been some controversy as to whether the magnetic fields of vertical threads seen in quiescent prominences are predominantly vertical or horizontal. We report finding special patterns of flow in a quiescent prominence observed by the Solar Optical Telescope aboard Hinode. This prominence is a small hedgerow prominence composed of many ver…

2008 The Astrophysical Journal
Hinode 77
Initial Venus Express magnetic field observations of the Venus bow shock location at solar minimum
DOI: 10.1016/j.pss.2007.09.012 Bibcode: 2008P&SS...56..785Z

Barabash, S.; Russell, C. T.; Zhang, T. L. +10 more

In this study, magnetic field measurements obtained by the Venus Express spacecraft are used to determine the bow shock position at solar minimum. The best fit of bow shock location from solar zenith angle 20-120° gives a terminator bow shock location of 2.14 RV (1 RV=6052 km) which is 1600 km closer to Venus than the 2.40 R<…

2008 Planetary and Space Science
VenusExpress 77
The early expansion of cluster cores
DOI: 10.1111/j.1365-2966.2008.13547.x Bibcode: 2008MNRAS.389..223B

Bastian, N.; Smith, L. J.; Goodwin, S. P. +4 more

The observed properties of young star clusters, such as the core radius and luminosity profile, change rapidly during the early evolution of the clusters. Here we present observations of six young clusters in M51 where we derive their sizes using Hubble Space Telescope (HST) imaging and ages using deep Gemini-North spectroscopy. We find evidence f…

2008 Monthly Notices of the Royal Astronomical Society
eHST 76
Spectropolarimetric Observation of an Emerging Flux Region: Triggering Mechanisms of Ellerman Bombs
DOI: 10.1086/590234 Bibcode: 2008ApJ...684..736W

Shibata, K.; Ueno, S.; Kitai, R. +6 more

A high spatial resolution observation of an emerging flux region (EFR) was made using a vector magnetograph and a Hα Lyot filtergraph with the Domeless Solar Telescope at Hida Observatory on 2006 October 22. In Hα wing images, we could see many Ellerman bombs (EBs) in the EFR. Observations in two modes, slit scan and slit fixed, were performed wit…

2008 The Astrophysical Journal
SOHO 76
The Stellar Mass Distribution in the Giant Star Forming Region NGC 346
DOI: 10.1088/0004-6256/135/1/173 Bibcode: 2008AJ....135..173S

Tosi, M.; Sabbi, E.; Nota, A. +8 more

Deep F555W and F814W Hubble Space Telescope (HST ) Advanced Camera for Survey (ACS) images are the basis for a study of the present-day mass function (PDMF) of NGC 346, the largest active star-forming region in the Small Magellanic Cloud (SMC). We find a PDMF slope of Γ = -1.43 ± 0.18 in the mass range 0.8-60 Msun, in excellent agreemen…

2008 The Astronomical Journal
eHST 76
Molecular Gas in NUclei of GAlaxies (NUGA). IX. The decoupled bars and gas inflow in NGC 2782
DOI: 10.1051/0004-6361:20078874 Bibcode: 2008A&A...482..133H

Tacconi, L. J.; Hunt, L. K.; Krips, M. +8 more

We present CO(1-0) and CO(2-1) maps of the starburst/Seyfert 1 galaxy NGC 2782 obtained with the IRAM interferometer, at 2.1 arcsec×1.5 arcsec and 0.7 arcsec×0.6 arcsec resolution respectively. The CO emission is aligned along the stellar nuclear bar of radius ~1 kpc, configured in an elongated structure with two spiral arms at high pitch angle ~9…

2008 Astronomy and Astrophysics
eHST 76
Circumstellar water vapour in M-type AGB stars: radiative transfer models, abundances, and predictions for HIFI
DOI: 10.1051/0004-6361:20078680 Bibcode: 2008A&A...479..779M

Olofsson, H.; Schöier, F. L.; Bergman, P. +2 more

Context: Surprisingly high amounts of H2O have recently been reported in the circumstellar envelope around the M-type asymptotic giant branch star W Hya. This has lead to the speculation that evaporation of icy cometary or planetary bodies might be an effective ongoing mechanism in such systems. However, substantial uncertainties remain, as the re…

2008 Astronomy and Astrophysics
ISO 76
A microlensing study of the accretion disc in the quasar MG 0414+0534
DOI: 10.1111/j.1365-2966.2008.14020.x Bibcode: 2008MNRAS.391.1955B

Wyithe, J. S. B.; Bate, N. F.; Floyd, D. J. E. +1 more

Observations of gravitational microlensing in multiply imaged quasars currently provide the only direct probe of quasar emission region structure on submicroarcsecond scales. The analyses of microlensing variability are observationally expensive, requiring long-term monitoring of lensed systems. Here, we demonstrate a technique for constraining th…

2008 Monthly Notices of the Royal Astronomical Society
eHST 76
Distribution and escape of molecular hydrogen in Titan's thermosphere and exosphere
DOI: 10.1029/2007JE003032 Bibcode: 2008JGRE..11310004C

Yelle, R. V.; Volk, K.; Cui, J.

We present an in-depth study of the distribution and escape of molecular hydrogen (H2) on Titan, based on the global average H2 distribution at altitudes between 1000 and 6000 km, extracted from a large sample of Cassini/Ion and Neutral Mass Spectrometer (INMS) measurements. Below Titan's exobase, the observed H2 d…

2008 Journal of Geophysical Research (Planets)
Cassini 76