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Smart Reasoning:

C&E

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Qaagi - Book of Why

Causes

Effects

about the star in 1983 when the Infrared Astronomical Satellite ( IRAS ) observed it(passive) was discoveredAn infrared excess

an asteroid belt within 1 au ( the Sun - Earth distance(passive) possibly caused byan infrared excess

nearby sources , a hidden companion , or dust emission(passive) might be caused byan infrared excess

The presence of dustalso causesan infrared excess

the interstellar dustcausingan infrared excess

warm dust(passive) caused byinfrared excesses

exozodiacal dust(passive) caused byan infrared excess

a circumstellar envelope ( CSE(passive) is ... caused byan infrared excess

a fraction of the gas ... dustcausesan infrared excess

dust grains in orbit around the star ( Aumann 1985(passive) caused byan infrared excess

warm ( ~500 K ) circumstellar dust(passive) caused bymid - infrared excess

circumstellar dust created in a stellar windcausesinfrared excess

their circumstellar dust shells ( Jura 1986(passive) caused byan infrared excess

a detached primordial dust shell around the giant(passive) to be caused bythe infrared excess

around the star by the Infrared Space Observatory(passive) was discoveredAn infrared excess

This light radiated by the structurewould createan infrared excess

the presence of protostellar disks(passive) caused byinfrared excesses

the wide component(passive) caused byan infrared excess

iron grains ( cf(passive) is caused bythe infrared excess

The more dense shellscausegreater infrared excess

warm circumstellar material(passive) caused byinfrared excess

warm disks(passive) caused bythe infrared excess

natural circurnstellar material(passive) caused byan infrared excess

minimum companion masses obtained from the radial velocity curve higher than dM masseswould causean infrared excess

a planetary scale hypervelocity impact(passive) was created bythe infrared excess

a centro - symmetric disk that only creates a signature in the square visibilities ( and(passive) caused byan infrared excess

the minimum companion mass ... a non - degenerate companionwould causean infrared excess

discs around young stars with the age of the system(passive) caused bythe infrared - excess

a circumstellar debris disk as pictured above(passive) caused byan infrared excess

a magma ocean planet or a circumplanetary disk or torus(passive) being created bythe infrared excess

Zuckerman et al(passive) was discovered byAn infrared excess

minimum companion masses derived from the RV - curve well below the masswould causean infrared excess

the circumstellar material that is common around very young stellar objects(passive) caused bythe near - infrared excess

mass loss(passive) caused byinfrared excess

an interstellar envelope ... Physicist Freeman Dyson 's photospherewould causean infrared excess

an interstellar envelope due to gas ejected from his photospherewould causean infrared excess

an interstellar envelope ... his photospherewould causean infrared excess

from a third companion in a wide orbit , which makes this system the second candidate hierarchical triple system containing an sdB staroriginatesfrom a third companion in a wide orbit , which makes this system the second candidate hierarchical triple system containing an sdB star

cancercan causecancer

in circumstellar disksdo ... originatein circumstellar disks

associated with the white dwarf G29 - 38 / mwas discoveredassociated with the white dwarf G29 - 38 / m

from the thermal emission of dust grains , which is linked to the presence of a stellar windoriginatingfrom the thermal emission of dust grains , which is linked to the presence of a stellar wind

they reasonedmust resultthey reasoned

to the H- and K - band fluxcontributingto the H- and K - band flux

their infrared colors to be different from the diskless Class III objectscausestheir infrared colors to be different from the diskless Class III objects

around G29 - 38discoveredaround G29 - 38

from a circumstellar - diskresultsfrom a circumstellar - disk

Blob

Smart Reasoning:

C&E

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