The Census of High- and Medium-mass Protostars (CHaMP) is the firstlarge-scale, unbiased, uniform mapping survey at sub-parsec scale resolution of90 GHz line emission from massive molecular clumps in the Milky Way. We presentthe first Mopra (ATNF) maps of the CHaMP survey region (300{\deg...
The prospect of detecting the first galaxies by observing their impact on the intergalactic medium (IGM) as they reionized it during the first billion years leads us to ask whether such indirect observations are capable of diagnosing which types of galaxies were most responsible for reionization. ...
The Census of High- and Medium-mass Protostars (CHaMP) is the first large-scale, unbiased, uniform mapping survey at sub-parsec-scale resolution of 90?GHz line emission from massive molecular clumps in the Milky Way. We present the first Mopra (ATNF) maps of the CHaMP survey region (300...
Stars with an initial mass on the Zero Age Main Sequence above 8 M⊙are considered to be high mass stars. They evolve in a short timescale (<25 Myr) by nuclear fusion of successively all available...Prantzos, NikosSpringer Berlin Heidelberg...
WMass Boys Hockey Stats Leaders: Two players finish with hat tricks Peyton Doyle|Jan 22, 2025 Subscriber Key that denotes Subscriber Exclusive content. WMass Boys Hockey Roundup: Ethan Mooney brings Amherst all the way back in OT Jason Asvestopoulos|Jan 22, 2025 ...
The development of the digital economy and advancements of new technology are expected to bring more opportunities to small and medium enterprises, or SMEs, through globalization on an electronic world trade platform. Chinese economy shows firming signs amid restructuring efforts A slew of upbeat econom...
High-energy astrophysics is the study of the processes that occur within stars, black holes and supernovae. These processes can be monitored by measuring the high-energy electromagnetic radiation and particles that they emit including x-rays, ultraviolet light and gamma rays. These observations are...
stars: individual (X Per, Vela X-1, V725 Tau, GX 301-2, SAX J0635.2+0533, V830 Censtars: neutronDetermining the type of matter that is inside a neutron star (NS) has been a long-standing goal of astrophysics. Despite this, most of the NS equations of state (EOS) that predict ...
Polnarev, Radiation of gravitational waves by a cluster of superdense stars, Sov. Astron. Lett. 18 (1974) 17. V.B. Braginsky and L.P. Grishchuk, Kinematic Resonance and Memory Effect in Free Mass Gravitational Antennas, Sov. Phys. JETP 62 (1985) 427 [INSPIRE]. V.B. Braginsky and K...
The starless condensations are colder than the star-forming cores, but the gas temperature across the whole protocluster is higher (by a factor of 1.3-1.5) than that measured typically in both infrared dark clouds and low-mass protoclusters. The non-thermal contributi...