Global star formation in the Milky Way from the VIALACTEA
... Traficante, L. Testi, Cesaroni R., G. Umana, F. Strafella, M. Brescia, M. Molinaro & Hi-GAL/VIALACTEA Team ...
... Traficante, L. Testi, Cesaroni R., G. Umana, F. Strafella, M. Brescia, M. Molinaro & Hi-GAL/VIALACTEA Team ...
Celebrating the centennial of a celestial yardstick
... offered was an indoor position as a computer. “I should be willing to pay thirty cents an hour in view of the quality of your work,” Pickering wrote, “although our usual price, in such cases, is twenty five cents an hour.” Leavitt, in accepting the position, referred to Pickering’s offer as “very li ...
... offered was an indoor position as a computer. “I should be willing to pay thirty cents an hour in view of the quality of your work,” Pickering wrote, “although our usual price, in such cases, is twenty five cents an hour.” Leavitt, in accepting the position, referred to Pickering’s offer as “very li ...
Session 2 - Early Autum Sky
... the constellation Sagittarius (where Jupiter is currently located now in fall of 2008), up through the northwest toward Cassiopeia. This glow will be brightest in Sagittarius, but still very noticeable in Aquila and Cygnus. The glow is caused by millions of stars which are part of our galaxy. Indivi ...
... the constellation Sagittarius (where Jupiter is currently located now in fall of 2008), up through the northwest toward Cassiopeia. This glow will be brightest in Sagittarius, but still very noticeable in Aquila and Cygnus. The glow is caused by millions of stars which are part of our galaxy. Indivi ...
Earth in Space - Learning Outcomes
... 13. A white dwarf star has a radius of 8000 km and a mass of 1.2 solar masses. (a) Calculate the density of the star in kg m-3. (b) Find the gravitational potential at a point on the surface. (c) Calculate the acceleration due to gravity at a point on the surface. (d) Estimate the potential energy ...
... 13. A white dwarf star has a radius of 8000 km and a mass of 1.2 solar masses. (a) Calculate the density of the star in kg m-3. (b) Find the gravitational potential at a point on the surface. (c) Calculate the acceleration due to gravity at a point on the surface. (d) Estimate the potential energy ...
ASTROPHYSICS UNIVERSE - Physics
... Once you know its luminosity you can know how far away it is (more on this ...
... Once you know its luminosity you can know how far away it is (more on this ...
"Stars" pdf file
... This is why stars have very large masses. The sun’s diameter is 1,4 million km long, 100 times more than the earth’s. But the sun is an average star. Star diameters range from a few hundredths to hundreds of times the solar one. Yet even star dimensions, no matter how large, are small compared to th ...
... This is why stars have very large masses. The sun’s diameter is 1,4 million km long, 100 times more than the earth’s. But the sun is an average star. Star diameters range from a few hundredths to hundreds of times the solar one. Yet even star dimensions, no matter how large, are small compared to th ...
Fulltext PDF
... The process of formation of a star can be divided into three phases. The first, known as 'star formation', involves massive interstellar clouds or cloud fragments, which have cooled to the point where they are detectable in molecular lines (such as CO) but which are unable to collapse because of an ...
... The process of formation of a star can be divided into three phases. The first, known as 'star formation', involves massive interstellar clouds or cloud fragments, which have cooled to the point where they are detectable in molecular lines (such as CO) but which are unable to collapse because of an ...
Syllabus - University of Texas Rio Grande Valley
... where in our galaxy we are likely to find open clusters. State how the position of the center of the Milky Way was determined. State approximate position of our Sun within the Milky Way. State the observational evidence that supports the Protogalactic Cloud Model for the formation of the Milky Way. ...
... where in our galaxy we are likely to find open clusters. State how the position of the center of the Milky Way was determined. State approximate position of our Sun within the Milky Way. State the observational evidence that supports the Protogalactic Cloud Model for the formation of the Milky Way. ...
005 Astrophysics problems
... 13. A white dwarf star has a radius of 8000 km and a mass of 1.2 solar masses. (a) Calculate the density of the star in kg m-3. (b) Find the gravitational potential at a point on the surface. (c) Calculate the acceleration due to gravity at a point on the surface. (d) Estimate the potential energy ...
... 13. A white dwarf star has a radius of 8000 km and a mass of 1.2 solar masses. (a) Calculate the density of the star in kg m-3. (b) Find the gravitational potential at a point on the surface. (c) Calculate the acceleration due to gravity at a point on the surface. (d) Estimate the potential energy ...
Evolution of Stars
... After He flash, temperature and luminosity depend on how much mass the star lost as it “climbed” the red giant branch Core gets enough mass that temperature reaches He fusion limit. Luminosity drops as equilibrium starts again. Core supported by He to C fusion. Rest of star supported by radiation an ...
... After He flash, temperature and luminosity depend on how much mass the star lost as it “climbed” the red giant branch Core gets enough mass that temperature reaches He fusion limit. Luminosity drops as equilibrium starts again. Core supported by He to C fusion. Rest of star supported by radiation an ...
Final Review Sheet
... in the future. Its radius is gradually increasing, but it is getting denser in its center. V. Post Main Sequence Evolution of Stars Lighter than 8 Msun Hydrogen fuel exhausted in inner 10 - 15% of mass. Helium core contracts and grows hotter. Hydrogen continues to burn in an overlying shell that is ...
... in the future. Its radius is gradually increasing, but it is getting denser in its center. V. Post Main Sequence Evolution of Stars Lighter than 8 Msun Hydrogen fuel exhausted in inner 10 - 15% of mass. Helium core contracts and grows hotter. Hydrogen continues to burn in an overlying shell that is ...
Activity 1: The Scientific Method
... 1) Start by becoming aware of your own biases. Do you believe any of the data is correlated? If so how? Relationship Example: radial motion of the stars and temperature Should state relationships that you believe might exist ...
... 1) Start by becoming aware of your own biases. Do you believe any of the data is correlated? If so how? Relationship Example: radial motion of the stars and temperature Should state relationships that you believe might exist ...
Lab PDF - NMSU Astronomy
... regardless of their luminosity or surface temperature, will lie along this line. In which corner of the diagram (upper right, upper left, lower right, or lower left) would stars with radii 1000 times larger than that of the Sun be plotted? In which corner would stars with radii 1000 times smaller th ...
... regardless of their luminosity or surface temperature, will lie along this line. In which corner of the diagram (upper right, upper left, lower right, or lower left) would stars with radii 1000 times larger than that of the Sun be plotted? In which corner would stars with radii 1000 times smaller th ...
Set 2: Nature of Galaxies
... • Non-constancy of the Ωlp will still cause winding but of the pattern and typically at a slower rate for (1, 2). • Where the local pattern speed matches the global pattern speed Lindblad resonances occur where the epicyclic amplitude increases due to forcing from the local density enhancement - can ...
... • Non-constancy of the Ωlp will still cause winding but of the pattern and typically at a slower rate for (1, 2). • Where the local pattern speed matches the global pattern speed Lindblad resonances occur where the epicyclic amplitude increases due to forcing from the local density enhancement - can ...
The Sky Viewed from Earth - Beck-Shop
... 3 Do all civilizations recognize the same constellations? Today, we have no problem knowing what day and month it is. We have calendars, watches, newspapers, television, computers, and Internet to keep us informed. But what about 4000 years ago? Back then, there was only the sky . . . Knowing one’s ...
... 3 Do all civilizations recognize the same constellations? Today, we have no problem knowing what day and month it is. We have calendars, watches, newspapers, television, computers, and Internet to keep us informed. But what about 4000 years ago? Back then, there was only the sky . . . Knowing one’s ...
Distant galaxies and quasars The ages of things Light
... estimate the total rate of star formation in the Universe (regardless which galaxies it is taking place in ... This, like the quasar evolution, shows a dramatic peak at earlier times ... but somewhat later than the quasars ...
... estimate the total rate of star formation in the Universe (regardless which galaxies it is taking place in ... This, like the quasar evolution, shows a dramatic peak at earlier times ... but somewhat later than the quasars ...
11 Stellar Remnants - Journigan-wiki
... The actual matter is passed through a mass transfer stream. Where this stream passes from the meeting Roche Lobes is called the LaGrange Point. The LaGrange Point is a point of gravitational neutrality where the influence of each star counteracts the gravitational force of its companion. To pass the ...
... The actual matter is passed through a mass transfer stream. Where this stream passes from the meeting Roche Lobes is called the LaGrange Point. The LaGrange Point is a point of gravitational neutrality where the influence of each star counteracts the gravitational force of its companion. To pass the ...
The Life and Times of a Neutron Star
... Exotic neutron stars may not be so rare. • Highly magnetized neutron stars may be as common as standard radio pulsars, but they don’t radio out their locations so they are harder to find. ...
... Exotic neutron stars may not be so rare. • Highly magnetized neutron stars may be as common as standard radio pulsars, but they don’t radio out their locations so they are harder to find. ...
Lecture 10: Stellar Evolution
... Energy and neutrons released in supernova explosion enable elements heavier than iron to form, including Au and U ...
... Energy and neutrons released in supernova explosion enable elements heavier than iron to form, including Au and U ...
Perseus (constellation)
Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.