Search Publications

Graphene oxide nanoparticles in the interstellar medium
DOI: 10.1093/mnrasl/slz131 Bibcode: 2019MNRAS.490L..17S

Sarre, P. J.

Dust particles play a major role in the formation, evolution and chemistry of interstellar clouds, stars, and planetary systems. Commonly identified forms include amorphous and crystalline carbon-rich particles and silicates. Also present in many astrophysical environments are polycyclic aromatic hydrocarbons (PAHs), detected through their infrare…

2019 Monthly Notices of the Royal Astronomical Society
ISO 13
Resolving the Interstellar Medium in Ultraluminous Infrared QSO Hosts with ALMA
DOI: 10.3847/1538-4357/ab50be Bibcode: 2019ApJ...887...24T

Kohno, Kotaro; Daddi, Emanuele; Gao, Yu +8 more

We present ALMA observations of the CO(1-0) line and 3 mm continuum emission in eight ultraluminous infrared (IR) quasi-stellar objects (QSOs) at z = 0.06-0.19. All eight IR QSO hosts are clearly resolved in their CO molecular gas emission with a median source size of 3.2 kpc, and seven out of eight sources are detected in 3 mm continuum, which is…

2019 The Astrophysical Journal
eHST 13
Compact star-forming galaxies preferentially quenched to become PSBs in z < 1 clusters
DOI: 10.1093/mnras/sty2840 Bibcode: 2019MNRAS.482.1640S

Simpson, Chris; Wild, Vivienne; Almaini, Omar +5 more

We analyse the structure of galaxies with high specific star formation rate (SSFR) in cluster and field environments in the redshift range 0.5 < z < 1.0. Recent studies have shown that these galaxies are strongly depleted in dense environments due to rapid environmental quenching, giving rise to post-starburst galaxies (PSBs). We use effecti…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
HST/COS Observations of the Warm Ionized Gaseous Halo of NGC 891
DOI: 10.3847/1538-4357/ab17df Bibcode: 2019ApJ...876..101Q

Bregman, Joel N.; Qu, Zhijie; Hodges-Kluck, Edmund J.

The metallicity of galactic gaseous halos provides insights into accretion and feedback of galaxies. The nearby edge-on galaxy NGC 891 has a multicomponent gaseous halo and a background active galactic nucleus (AGN; LQAC 035+042 003) projected 5 kpc above the disk near the minor axis. Against the UV continuum of this AGN, we detect lines from 13 i…

2019 The Astrophysical Journal
eHST 13
Discovery statistics and 1/a distribution of long-period comets detected during 1801-2017
DOI: 10.1093/mnras/stz025 Bibcode: 2019MNRAS.484.3463K

Dybczyński, Piotr A.; Królikowska, Małgorzata

For the last two decades, we have been observing a huge increase in discoveries of long-period comets (LPCs), especially those with large perihelion distances. We collected data for a full sample of LPCs discovered during 1801-2017, including their osculating orbits, discovery moments (to study the discovery distances) and original semimajor axes …

2019 Monthly Notices of the Royal Astronomical Society
SOHO 13
New luminous blue variable candidates in NGC 4736
DOI: 10.1093/mnrasl/sly241 Bibcode: 2019MNRAS.484L..24S

Vinokurov, A.; Solovyeva, Y.; Atapin, K. +8 more

We have found three new luminous blue variable (LBV) candidates in the star-forming galaxy NGC 4736. They show typical well-known LBV spectra, broad and strong hydrogen lines, He I lines, many Fe II lines, and forbidden [Fe II] and [Fe III]. Using archival Hubble Space Telescope and ground-based telescope data, we have estimated the bolometric mag…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
Star formation in far-IR AGN and non-AGN galaxies in the green valley - II. Morphological analysis
DOI: 10.1093/mnras/stz434 Bibcode: 2019MNRAS.485..452M

Pović, Mirjana; Väisänen, Petri; Mahoro, Antoine +2 more

This paper studies morphological properties of 103 green valley FIR active and 2609 non-active galaxies presented in Mahoro, Pović & Nkundabakura (2017). The photometric data from the COSMOS survey were used, and the morphological parameters, such as Abraham and Conselice-Bershady concentration indices, Gini, M20 moment of light, and asymmetry…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
Chemical analysis of K giants in the young open cluster NGC 2345
DOI: 10.1093/mnras/sty2991 Bibcode: 2019MNRAS.482.5275H

Pereira, C. B.; Holanda, N.; Drake, N. A.

We present results for the elemental abundances of five K giants of the young open cluster NGC 2345. The atmospheric parameters of the studied giants and their chemical abundances were determined using high-resolution optical spectroscopy. In this study, we determine abundances of light elements (Li, C, N), light odd-Z elements (Na, Al), α-element…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 13
Detailed study of the Milky Way globular cluster Laevens 3
DOI: 10.1093/mnras/stz2592 Bibcode: 2019MNRAS.490.1498L

Martin, Nicolas; Ibata, Rodrigo A.; Mackey, Dougal +4 more

We present a photometric and spectroscopic study of the Milky Way satellite Laevens 3. Using MegaCam/Canada-France-Hawaii Telescope g and i photometry and Keck II/DEIMOS multi-object spectroscopy, we refine the structural and stellar properties of the system. The Laevens 3 colour-magnitude diagram shows that it is quite metal-poor, old (13.0 ± 1.0…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 13
Surface evolution of the Anhur region on comet 67P/Churyumov-Gerasimenko from high-resolution OSIRIS images
DOI: 10.1051/0004-6361/201834824 Bibcode: 2019A&A...630A..13F

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +34 more

Context. The southern hemisphere of comet 67P/Churyumov-Gerasimenko (67P) became observable by the Rosetta mission in March 2015, a few months before cometary southern vernal equinox. The Anhur region in the southern part of the comet's larger lobe was found to be highly eroded, enriched in volatiles, and highly active.
Aims: We analyze high-…

2019 Astronomy and Astrophysics
Rosetta 13