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Here I describe recent studies of objects with molecular hydrogen emission that is strong relative to other spectral lines. Large telescopes and fast spectrometers have made the 2 {\mu}m window accessible even for relatively faint objects.…

宇宙学与河外天体物理 · 物理学 2011-07-25 Gary J. Ferland

We present results of optical-UV observations of the 200 Myr old rotation-powered radio pulsar J0108$-$1431 with the Hubble Space Telescope. We found a putative candidate for the far-UV (FUV) pulsar counterpart, with the flux density $f_\nu…

高能天体物理现象 · 物理学 2021-04-14 Vadim Abramkin , Yuriy Shibanov , Roberto P. Mignani , George G. Pavlov

We continue to see a range of values for the Hubble constant obtained from gravitationally lensed multiple image time delays when assuming an isothermal lens despite a robust value from the HST key project (72 +- 8 km s^-1 Mpc^-1. One…

天体物理学 · 物理学 2008-11-26 Benjamin M. Dobke , Lindsay J. King , Michael Fellhauer

The European Space Agency Rosetta/Philae mission to Comet 67P/Churyumov-Gerasimenko in 2014-2016 is the most complete and diverse investigation of a comet carried out thus far. Yet, many physical and chemical properties of the comet remain…

地球与行星天体物理 · 物理学 2022-09-14 Björn J. R. Davidsson , Nalin H. Samarasinha , Davide Farnocchia , Pedro J. Gutiérrez

Neutron stars cooling passively since their birth may be reheated in their late-stage evolution by a number of possible phenomena: rotochemical, vortex creep, crust cracking, magnetic field decay, or more exotic processes such as removal of…

高能天体物理现象 · 物理学 2024-03-13 Nirmal Raj , Prajwal Shivanna , Gaurav Niraj Rachh

We investigate the thermal evolution of 3I/ATLAS, the third macroscopic interstellar object discovered on 2025 July 1. By comparing modeled thermal profiles with observations of volatile activity, it is possible to constrain bulk physical…

地球与行星天体物理 · 物理学 2026-01-22 Atsuhiro Yaginuma , Aster G. Taylor , Darryl Z. Seligman

We monitored the chromospheric activity in the Ca II H & K lines of 13 solar-type stars (including the Sun); 8 of them over three years at the CFHT and 5 in a single run at the VLT. Ten of the 13 targets have close planetary companions. All…

天体物理学 · 物理学 2009-11-10 E. Shkolnik , G. A. H. Walker , D. A. Bohlender , P. -G. Gu , M. Kürster

Vibration-rotation lines of H$_{2}$ from highly excited levels approaching the dissociation limit have been detected at a number of locations in the shocked gas of the Orion Molecular Cloud (OMC-1), including in a Herbig-Haro object near…

星系天体物理 · 物理学 2017-03-15 T. R. Geballe , M. G. Burton , R. E. Pike

Context. Near-Earth asteroid-comet transition object 107P/ (4015) Wilson-Harrington is a possible target of the joint European Space Agency (ESA) and Japanese Aerospace Exploration Agency (JAXA) Marco Polo sample return mission. Physical…

We report the discovery of recurrent activity on quasi-Hilda comet (QHC) 362P/(457175) 2008 GO98. The first activity epoch was discovered during the perihelion passage of 362P. The first activity epoch was discovered during the perihelion…

High resolution imaging is an important tool for follow-up study of exoplanet candidates found via transit detection with the Kepler Mission. We discuss here HST imaging with the WFC3 of 23 stars that host particularly interesting Kepler…

地球与行星天体物理 · 物理学 2015-06-22 Ronald L. Gilliland , Kimberly M. S. Cartier , Elisabeth R. Adams , David R. Ciardi , Paul Kalas , Jason T. Wright

Context: Trans-Neptunian objects are distant bodies that retain valuable information about the origin and evolution of the Solar System. Many of these objects constitute binary systems. Studying binaries allows us to further characterise…

地球与行星天体物理 · 物理学 2026-05-22 J. M. Gómez-Limón , R. Leiva , J. L. Ortiz , P. Santos-Sanz , M. Kretlow , Y. Kilic , J. L. Rizos , A. Álvarez-Candal , T. G. Müller

We present the results of a multi-line and continuum study towards the source IRAS 23385+6053,performed with the IRAM-30m telescope, the Plateau de Bure Interferometer, the Very Large Array Interferometer and the James Clerk Maxwell…

天体物理学 · 物理学 2009-11-10 F. Fontani , R. Cesaroni , L. Testi , C. M. Walmsley , S. Molinari , R. Neri , D. Shepherd , J. Brand , F. Palla , Q. Zhang

By coupling observations of type Ia supernovae with results obtained from the best available numerical models we constrain the Hubble constant, independently of any external calibrators. We find an absolute lower limit of Ho > 50 km/s/Mpc.…

天体物理学 · 物理学 2009-11-10 M. Stritzinger , B. Leibundgut

We have acquired high-resolution echelle spectra of 225 F6-M5 type stars in the southern hemisphere. The stars are targets or candidates to be targets for the Anglo-Australian Planet Search. CaII HK line cores were used to derive activity…

For the first time, spectral signs of subtle coma activity were observed simultaneously on four main-belt primitive asteroids (145) Adeona, (704) Interamnia, (779) Nina, and (1474) Beira around their perihelion distances in September 2012,…

地球与行星天体物理 · 物理学 2017-12-11 Vladimir V. Busarev , Andrei B. Makalkin , Faith Vilas , Sergey I. Barabanov , Marina P. Scherbina

We present observations of far-infrared (50-200 micron) OH and H2O emission of the disk around the Herbig Ae star HD 163296 obtained with Herschel/PACS in the context of the DIGIT key program. In addition to strong [OI] emission, a number…

太阳与恒星天体物理 · 物理学 2015-06-05 D. Fedele , S. Bruderer , E. F. van Dishoeck , G. J. Herczeg , N. J. Evans , J. Bouwman , Th. Henning , J. Green

For near-Sun missions, the spacecraft approaches very close to the Sun and space environmental effects become relevant. Strong restrictions on how much close it can get derive from the maximum temperature that the used materials can stand,…

空间物理 · 物理学 2017-10-25 Elena Ancona , Roman Ya. Kezerashvili

Jupiters south polar region was observed by JWST Mid Infrared Instrument in December 2022. We used the Medium Resolution Spectrometer mode to provide new information about Jupiters South Polar stratosphere. The southern auroral region was…