Search results for "Atacama Large Millimeter Array"

showing 2 items of 2 documents

ALMA full polarization observations of PKS1830-211 during its record-breaking flare of 2019

2020

We report Atacama Large Millimeter Array (ALMA) Band 6 full-polarization observations of the lensed blazar PKS 1830-211 during its record-breaking radio and gamma-ray flare in the spring of 2019. The observations were taken close to the peak of the gamma activity and show a clear difference in polarization state between the two time-delayed images. The leading image has a fractional polarization about three times lower than the trailing image, implying that significant depolarization occurred during the flare. In addition, we observe clear intra-hour variability of the polarization properties between the two lensed images, with a quasi-linear increase in the differential electric-vector pos…

Astrophysics::High Energy Astrophysical PhenomenaGamma rays: generalgeneral [Gamma rays]FOS: Physical sciencesQuasars: individual: PKS1830-211AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionlawPolarization0103 physical sciencesindividual: PKS1830-211 [Quasars]Blazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsQuasarAtacama Large Millimeter ArrayPolarization (waves)Position angleFractional polarizationSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaFlare
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Carbon Monoxide in the Cold Debris of Supernova 1987A

2013

We report spectroscopic and imaging observations of rotational transitions of cold CO and SiO in the ejecta of SN1987A, the first such emission detected in a supernova remnant. In addition to line luminosities for the CO J=1-0, 2-1, 6-5, and 7-6 transitions, we present upper limits for all other transitions up to J=13-12, collectively measured from the Atacama Large Millimeter Array (ALMA), the Atacama Pathfinder EXperiment (APEX), and the Herschel Spectral and Photometric Imaging REceiver (SPIRE). Simple models show the lines are emitted from at least 0.01 solar masses of CO at a temperature > 14 K, confined within at most 35% of a spherical volume expanding at ~ 2000 km/s. Moreover, we…

FOS: Physical sciencesAstrophysicsWAVELENGTHindividual (SN1987A) [supernovae]FACILITYEjectaSupernova remnantSolar and Stellar Astrophysics (astro-ph.SR)3-DIMENSIONAL STRUCTURELine (formation)PhysicsSolar massSN-1987AINSTRUMENTsupernova remnants [ISM]Astronomy and AstrophysicsAtacama Large Millimeter ArrayDebrisSupernovaSpireEJECTACASSIOPEIAPhysics and AstronomyAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceREMNANTSN 1987A
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