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The Korean 1592--1593 Record of a Guest Star: Animpostor`of the
The Korean 1592--1593 Record of a Guest Star: Animpostor`of the

... might have been the Cas A SN event. On the other hand, Stephenson & Yau (1987) (see also Stephenson & Green 2002, for a summary), who studied this Korean record in detail, concluded that not only the date but also the positional agreement between the guest star and Cas A was poor, so that this Korea ...
A Walk through the Southern Sky: A Guide to Stars and
A Walk through the Southern Sky: A Guide to Stars and

A search for a new class of pulsating DA white dwarf stars in the DB
A search for a new class of pulsating DA white dwarf stars in the DB

Bez nadpisu
Bez nadpisu

Examining the M67 Classification as an Open Cluster
Examining the M67 Classification as an Open Cluster

... are indicated in the diagram by the blue color. As is seen, the color-magnitude diagram for M67 shows a short main sequence extending from  B - V   0.4 , where the turn-off point is located, up to  B - V   0.7 . After  B - V   0.7 it starts merging in the field region stars and is not seen ...
Mergers of massive main sequence binaries
Mergers of massive main sequence binaries

Table of Contents - Shawnee State University
Table of Contents - Shawnee State University

... - Winds between the Big and Little Dippers. - Generally takes up all of the remaining bright stars between those two constellations. - Draco’s head hangs down near Cepheus. - Draco is probably the toughest circumpolar constellation to find, - If you can find it, you could tell the ‘dragon heaven’ st ...
Epsilon Aurigae: a rare stellar eclipse - Project VS
Epsilon Aurigae: a rare stellar eclipse - Project VS

AAVSO: Epsilon Aurigae
AAVSO: Epsilon Aurigae

Cassiopeia Kelly Pearce
Cassiopeia Kelly Pearce

... within the boundary of the constellation. These observable objects include both New General Catalogue objects and Messier objects. New General Catalogue is a catalogue of recorded deep sky objects and is referred to as NGC (SEDS, The Messier Catalog, 2010). The first of these objects, NGC 457, is al ...
KINEMATIC DISCOVERY OF A STELLAR STREAM LOCATED IN
KINEMATIC DISCOVERY OF A STELLAR STREAM LOCATED IN

Protostellar/PMS Mass Infall Luminosity Problem
Protostellar/PMS Mass Infall Luminosity Problem

The Pleiades in the Salle des Taureaux", Grotte de Lascaux
The Pleiades in the Salle des Taureaux", Grotte de Lascaux

Hertzsprung–Russell diagram - Wikipedia, the free encyclopedia
Hertzsprung–Russell diagram - Wikipedia, the free encyclopedia

HR DIAGRAMS OF STAR CLUSTERS
HR DIAGRAMS OF STAR CLUSTERS

... sequence: since these are the stars that leave the main sequence first as the cluster ages, the “turnoff” point on the main-sequence is a critical function of the age of the cluster. You may not see many stars on the giant branch, since giant branch stars have relatively short life spans (about 10% ...
hr diagrams of star clusters
hr diagrams of star clusters

... sequence: since these are the stars that leave the main sequence first as the cluster ages, the “turnoff” point on the main-sequence is a critical function of the age of the cluster. You may not see many stars on the giant branch, since giant branch stars have relatively short life spans (about 10% ...
THE PERIOD OF ROTATION OF THE SUN
THE PERIOD OF ROTATION OF THE SUN

... sequence: since these are the stars that leave the main sequence first as the cluster ages, the “turnoff” point on the main-sequence is a critical function of the age of the cluster. You may not see many stars on the giant branch, since giant branch stars have relatively short life spans (about 10% ...
Absolute magnitudes and kinematics of barium
Absolute magnitudes and kinematics of barium

The first photometric analysis of the overcontact binary MQ UMa with
The first photometric analysis of the overcontact binary MQ UMa with

... ranges from A2V to K5V, and has a period from 0.2211 days to 1.1318 days. The sample has covered nearly all kinds of W UMa type contact binaries which means it is appropriate to MQ UMa. The period of MQ UMa is 0.476058 days, so the color index of J −K calculated by Equation (4) is 0.266 (±0.042), wh ...
PDF - Department of Statistics
PDF - Department of Statistics

Have You Seen Canopus Tonight?
Have You Seen Canopus Tonight?

... are familiar. Others know Polaris directs us north and no star is closer to our solar system than the Alpha Centauri system. Betelgeuse and Rigel help outline winter’s Orion while Vega, Deneb and Altair form the summer triangle. Regulus, heart of Leo the Lion, heralds spring, and Aldebaran follows t ...
Small star patterns for telescopes and binoculars Demelza Ramakers
Small star patterns for telescopes and binoculars Demelza Ramakers

... vary in magnitude from 7 to 9. In the middle is a bright star of magnitude 5 visible. The chain of stars lead to the open star cluster NGC 1502. Kemble’s Cascade is best viewed through binoculars because of its size. Take the first and last star from constellation Cassiopeia, the two ends of the ‘W’ ...
Annual report 2004 - Département d`Astrophysique, Géophysique et
Annual report 2004 - Département d`Astrophysique, Géophysique et

... LPVs on the orbital solution and resulted in an improved orbital period, a small, but significant, eccentricity (e=0.03), and stellar masses of 15 M and 3 M with corresponding radii of 8.3 R and 2.1 R , and temperatures of 25500 and 12500 K. In the course of 2004, the orbital and dimensional analysi ...
Red supergiants and the past of Cygnus OB2
Red supergiants and the past of Cygnus OB2

Star 1 A star is a massive, luminous ball of plasma held together by
Star 1 A star is a massive, luminous ball of plasma held together by

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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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