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The Perseus molecular cloud complex is a ~30pc long chain of molecular clouds most well-known for the two star-forming clusters NGC1333 and IC348 and the well-studied outflow source in B5. However, when studied at mid- to far-infrared…

天体物理学 · 物理学 2009-11-11 Naomi A. Ridge , Scott L. Schnee , Alyssa A. Goodman , Jonathan B. Foster

I review the literature covering the issue of interstellar extinction toward the Milky Way bulge, with emphasis placed on findings from planetary nebulae, RR Lyrae, and red clump stars. I also report on observations from HI gas and globular…

太阳与恒星天体物理 · 物理学 2016-07-06 David M. Nataf

Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the…

天体物理学 · 物理学 2008-04-01 Carl H. Gibson , Rudolph E. Schild

Data from the Five College Radio Astronomy Observatory CO Mapping Survey of the Taurus molecular cloud are combined with extinction data for a sample of 292 background field stars to investigate the uptake of CO from the gas to icy grain…

星系天体物理 · 物理学 2010-07-20 D. C. B. Whittet , P. F. Goldsmith , J. L. Pineda

The nature of the icy material accreted by comets during their formation in the outer regions of the protosolar nebula is a major open question in planetary science. Some scenarios of comet formation predict that these bodies agglomerated…

地球与行星天体物理 · 物理学 2016-05-04 O. Mousis , J. I. Lunine , A. Luspay-Kuti , T. Guillot , B. Marty , M. Ali-Dib , P. Wurz , K. Altwegg , A. Bieler , M. Hässig , M. Rubin , P. Vernazza , J. H. Waite

We explore the extinction properties of the dust in the distant universe through the afterglows of high-redshifted GRBs based on the "Drude" model which, unlike previous studies, does not require a prior assumption of template extinction…

天体物理学 · 物理学 2008-12-18 S. L. Liang , Aigen Li

(Abridged) We use 8 micron Spitzer GLIMPSE images to make extinction maps of 10 IRDCs, selected to be relatively nearby and massive. The extinction mapping technique requires modeling the IR background intensity behind the cloud, which is…

天体物理学 · 物理学 2011-02-11 Michael J. Butler , Jonathan C. Tan

High energy cosmic ray jets from nearby mergers or accretion induced collapse (AIC) of neutron stars (NS) that hit the atmosphere can produce lethal fluxes of atmospheric muons at ground level, underground and underwater, destroy the ozone…

天体物理学 · 物理学 2008-11-26 Arnon Dar , Ari Laor , Nir J. Shaviv

Large masses of absorbing material are inferred to exist in cooling flows in clusters of galaxies from the excess X-ray absorption in the spectra of some X-ray clusters. The absorbing material is probably in the form of cold clouds…

天体物理学 · 物理学 2009-10-31 A. C. S. Friaca , L. C. Jafelice

We do a preliminary modelling of the photosynthetic rates of phytoplankton at the very beginning of the Paleogene, just after the impact of the Chicxulub asteroid, which decisively contributed to the last known mass extinction of the…

地球与行星天体物理 · 物理学 2012-09-21 Noel Perez , Rolando Cardenas , Osmel Martin , Reinaldo Rojas

Recent spacecraft observations exploring solar system properties impact standard paradigms of the formation of stars, planets and comets. We stress the unexpected cloud of microscopic dust resulting from the DEEP IMPACT mission, and the…

宇宙学与河外天体物理 · 物理学 2010-12-30 Rudolph E. Schild , Carl H. Gibson

Glaciations were attributed to variations of the Earths orbit (Milankovitch cycles). But the best ever dated paleoclimatic record (from a speleothem from Devils Hole, Nevada) demonstrated that the end of the last glacial period (termination…

地球物理 · 物理学 2009-09-10 Yavor Y. Shopov , Diana A. Stoykova , Katerina Stoitchkova , Anton Tanev

Prompt cusps are the densest quasi-equilibrium dark matter objects; one forms at the instant of collapse within every isolated peak of the initial cosmological density field. They have power-law density profiles, $\rho \propto r^{-1.5}$…

宇宙学与河外天体物理 · 物理学 2023-05-03 Jens Stücker , Go Ogiya , Simon D. M. White , Raul E. Angulo

Edge Cloud 2 (EC2) is a molecular cloud, about 35 pc in size, with one of the largest galactocentric distances known to exist in the Milky Way. We present observations of a peak CO emission region in the cloud and use these to determine its…

天体物理学 · 物理学 2009-11-13 P. M. E. Ruffle , T. J. Millar , H. Roberts , D. A. Lubowich , C. Henkel , J. M. Pasachoff , G. Brammer , .

We construct a quasar extinction curve based on the blue and red composite quasar spectra of Richards et al. (2003) prepared from the SDSS survey. This extinction curve does not show any traces of the 2200 A feature characteristic of the…

天体物理学 · 物理学 2009-11-10 B. Czerny , J. Li , Z. Loska , R. Szczerba

Identification by the Ulysses spacecraft of interstellar grains inside the planetary system provides a new window for the study of diffuse interstellar matter. Dust particles observed by Ulysses and confirmed by Galileo are more massive…

天体物理学 · 物理学 2015-06-24 E. Grün , M. Landgraf

Neutral hydrogen (HI) emission closely traces the dust column density at high Galactic latitudes and is thus a powerful tool for predicting dust extinction. However, the relation between HI column density $N_{\rm HI}$ and high-latitude dust…

星系天体物理 · 物理学 2025-04-28 Yun-Ting Cheng , Brandon S. Hensley , Tzu-Ching Chang , Olivier Doré

The joint use of accurate near- and mid-infrared photometry from the 2MASS and WISE catalogues has allowed the variations of the extinction law and the dust grain size distribution in high Galactic latitudes (|b|>50) at distances up to 3…

星系天体物理 · 物理学 2019-10-25 George Gontcharov

Recently, an ionized cloud of gas was discovered plunging toward the supermassive black hole, SgrA*, at the centre of the Milky Way. The cloud is being tidally disrupted along its path to closest approach at ~3100 Schwarzschild radii from…

星系天体物理 · 物理学 2015-06-03 Ruth A. Murray-Clay , Abraham Loeb

Systems of close-in super-Earths display striking diversity in planetary bulk density and composition. Giant impacts are expected to play a role in the formation of many of these worlds. Previous works, focused on the mechanical shock…

地球与行星天体物理 · 物理学 2019-03-27 John B. Biersteker , Hilke E. Schlichting