Search Publications

Precise photometry and astrometry in the core of the globular cluster NGC 6121 using PSF-R techniques
DOI: 10.1117/12.2560938 Bibcode: 2020SPIE11448E..0GM

Tolstoy, Eline; Milli, Julien; Fiorentino, Giuliana +6 more

Precise stellar photometry and astrometry require the best possible modelling of the point spread function (PSF). To date, the best performances have been obtained when building the PSF a posteriori, meaning directly from the image of dense stellar fields, by exploiting the fact that each star represents a different realisation of the same PSF. Th…

2020 Adaptive Optics Systems VII
eHST 0
Subsurface ice on comet 67P is softer than candyfloss
DOI: 10.1016/S0262-4079(20)31962-X Bibcode: 2020NewSc.248Q..22C

Crane, Leah

2020 New Scientist
Rosetta 0
Report from ILEWG Task Groups: Science, Technology, human aspects, roadmaps, socio-economics, young lunar explorers, MoonVillage, MoonMars synergies, EuroMoonMars, ArtMoonMars
DOI: 10.5194/egusphere-egu2020-22025 Bibcode: 2020EGUGA..2222025F

Foing, Bernard

ILEWG has been organising since 1994 ICEUM International Conferences on Exploration & Utilisation of the Moon with published proceedings, and where community declarations have been prepared and endorsed by community participants. ILEWG has co-organised and co-sponsored lunar sessions at EGU, COSPAR, EPSC.ILEWG task groups include science, tech…

2020 EGU General Assembly Conference Abstracts
Chandrayaan-1 SMART-1 0
Herbig-Haro flows around the BBWo 192E (GM 1-23) nebula
DOI: 10.1093/mnras/staa2694 Bibcode: 2020MNRAS.498.5109M

Bally, J.; Rastorguev, A. S.; Movsessian, T. A. +2 more

Looking for evidence of recent star formation, we have studied a small comet-shaped reflection nebula, known as BBWo 192E (GM 1-23), which is located in the dark cloud SL 4 in the Vela Molecular Ridge cloud C, and a young infrared cluster embedded into the nebula. We obtained the images of BBWo 192E in Hα and [S II] lines and in a Sloan Digital Sk…

2020 Monthly Notices of the Royal Astronomical Society
AKARI Gaia 0
Kinematical structure of open clusters within 1 kpc by Gaia
Bibcode: 2020BlgAJ..32...83E

Elsanhoury, W. H.

The work is based on proper motions, radial velocities, and absolute magnitudes of 56 open clusters located within 1 kpc. We classify those as a function of their distances into five groups (Freedman and Diaconis's rule) as well as a double frequency table may be achieved. For these groups, we calculated their velocity ellipsoid parameters VEPs, e…

2020 Bulgarian Astronomical Journal
Gaia 0
Ammonium salts on comet 67P
DOI: 10.1126/science.367.6483.1207-l Bibcode: 2020Sci...367T1207S

Smith, Keith T.

2020 Science
Rosetta 0
Erratum: 'XMM-newton large program on SN1006 - II: Thermal emission' (2016, MNRAS, 462, 158)
DOI: 10.1093/mnras/staa2873 Bibcode: 2020MNRAS.499..862L

Vink, Jacco; Miceli, Marco; Bocchino, Fabrizio +2 more

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Comparative study of activity of the near-parabolic orbitcomet C/1977 R1 (Kohler)
Bibcode: 2020BAAA...61C..53D

de Almeida, A. A.; Sanzovo, G. C.; de Araújo, L. F.

Kohler is considered a case of young, nearly parabolic comet. In this work we deduce, semi-empirically, water and hydroxyl production rates from the photometric observations of this comet taken from the Archive of Photometric Data on Comets and British Astronomical Society archives. Our results are being compared with those obtained from radio obs…

2020 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
SOHO 0
Gaia DR2 and Serbian-Bulgarian investigations
Bibcode: 2020BlgAJ..33...31D

Damljanović, Goran

On April $25^{th}$ 2018, the second release of the Gaia catalog (DR2) appeared. It is based on 640 days of Gaia satellite observations; GAIA means Global Astrometric Interferometer for Astrophysics. The observing period was August $22^{nd}$ 2014 - May $23^{rd}$ 2016 (1.75 yr or 21 months with some interruptions). The reference epoch is J2015.5 . T…

2020 Bulgarian Astronomical Journal
Gaia 0
An AGB Star with a Thick Circumstellar Shell
DOI: 10.1088/1538-3873/ab77d8 Bibcode: 2020PASP..132d4201M

Wang, Lifan; Durré, Mark; Mould, Jeremy +1 more

The Asymptotic Giant Branch is the terminal phase of red giant evolution with timescales of millions of years and a total mass lost from the star that is a significant fraction of the initial mass. Investigation of one of these stars, WISEA J173046.10-344455.5, a kpc in the direction of the center of the Galaxy, reveals a cool oxygen rich star wit…

2020 Publications of the Astronomical Society of the Pacific
Gaia 0