* Astronomy

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Maxima of long period variable W Ophiuchi on the 12th March, 2010 Magnitude: 9.3-14.9 V Type: Mira Period: 332.68 days Position (2000): RA 16 21 24.46, Dec -07 42 00.2

Blobrana · Blobrana

Astronomers have discovered one of the closest stars to our Sun, and they say that more undetected close neighbours may be lurking in our vicinity. The new star was found because its relatively swift motion across the sky was picked up by automated sky surveys. It ranks as the third closest star syste...

Blobrana · Blobrana

Title: The mass and radius of the M-dwarf in the short period eclipsing binary RR Caeli Authors: P.F.L. Maxted (1,2), D. O'Donoghue (3), L. Morales-Rueda (4,2), R. Napiwotzki (5) ((1)Keele University, UK, (2)Southampton University, UK, (3) SAAO, South Africa, (4) Universi...

Blobrana · Blobrana

Title: Cool Young Stars in the Northern Hemisphere: Beta Pictoris and AB Doradus Moving Group Candidates Authors: Joshua E. Schlieder, Sébastien Lépine, Michal Simon As part of our continuing effort to identify new, low-mass members of nearby, young moving groups (NYMGs), we present a list of y...

Blobrana · Blobrana

Title: XMM-Newton observations of the low-mass X-ray binary XB1832-330 in the galactic globular cluster NGC 6652 Authors: L. Sidoli (1), N. La Palombara (1), T. Oosterbroek (2), A.N. Parmar (3) ((1)-INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica, Milano, Italy (2)-Science Payload a...

Blobrana · Blobrana

The dwarf nova QZ Virgo (= T Leo) is in outburst. Date: 2009 01 26 Magnitude: 10.2 - 15.7 Period: ? Satellite period: unknown Type: UGSU Position(2000): RA=11 38 26.82, Dec=+03°22'07.1"

Blobrana · Blobrana

Title: Rotten Egg Nebula: The magnetic field of a binary evolved star Authors: M. L. Leal-Ferreira, W. H. T. Vlemmings, P. J. Diamond, A. Kemball, N. Amiri, J.-F. Desmurs Most of PNe are not spherical. The loss of spherical symmetry occurs somewhere between the AGB and PN phase. The cause of this chan...

Blobrana · Blobrana

Maximum of U Herculis Variable Star, at 0.6h, 22nd February, 2010 Magnitude=6.4mag Minimum=13.4mag Period= 2.1days Position(2000): RA =16 25 47.4713, Dec =+18 53 32.867

Blobrana · Blobrana

Title: Massive star-formation toward G28.87+0.07 (IRAS 18411-0338) investigated by means of maser kinematics and radio to infrared, continuum observations Authors: J. J. Li, L. Moscadelli, R. Cesaroni, R. S. Furuya, Y. Xu, T. Usuda, K. M. Menten, M. Pestalozzi, D. Elia, E. Schisano We used the V...

Blobrana · Blobrana

UGPSJ0722-05 is a sub-brown dwarf located approximately nine light years from Earth. The astronomical object was discovered by Philip Lucas at the University of Hertfordshire in 2010. Read more

Blobrana · Blobrana

The grazing eclipsing dwarf nova CW Monocerotis is in outburst. Date: 27th October 2008 Magnitude: 11.9 - 16.3 Period: 121.7 days Satellite period: 0.1766 days Type: UGSS Position(2000): RA=06 36 54.58, Dec=+00°02'17.2"

Blobrana · Blobrana

Date of outbreak: 9th June 2010 Magnitude: 12.9 - 16.62 V Period: 0.2008 days Orbital period of satellite: days Type: UGZ Position(2000): RA=23 40 23.70, Dec=+12°37'41.7"

Blobrana · Blobrana

When stars like our sun die, they bloat to become red giants and then eject gigantic clouds of gas and dust into space. Increasingly, however, scientists found themselves at a profound loss to explain how exactly dying stars could blow away these clouds. Now astrophysicists propose that unexpecte...

Blobrana · Blobrana

Astronomers Release an Unprecedented Data Set on Variability of Celestial Objects An example of a star that flares occasionally. This is a so-called dwarf nova, a binary star system where a material flows from a red giant star to a compact, dense white dwarf companion, and sometimes causes major e...

Blobrana · Blobrana

Maxima of long period variable RT Sagittarii on the 29th April, 2010 Magnitude: 7.0-13.3 V Type: Mira Position (2000): RA 20 17 43.6461, Dec -39 06 46.024

	Sub Forum	Topics	Posts	Last Post
	Exoplanets Exoplanets	342	729	Dec 6 12:10 2017 by Blobrana
	Stars	1643	2761	Jun 10 15:01 2018 by Blobrana

Topic		Started By	Replies	Last Post
	W Ophiuchi (Preview) Maxima of long period variable W Ophiuchi on the 12th March, 2010 Magnitude: 9.3-14.9 V Type: Mira Period: 332.68 days Position (2000): RA 16 21 24.46, Dec -07 42 00.2	Blobrana	1	Jan 24 08:01 2012 by Blobrana
	Teegarden's Star Star (Preview) Astronomers have discovered one of the closest stars to our Sun, and they say that more undetected close neighbours may be lurking in our vicinity. The new star was found because its relatively swift motion across the sky was picked up by automated sky surveys. It ranks as the third closest star syste...	Blobrana	1	Jan 23 07:14 2012 by Blobrana
	RR Caeli (Preview) Title: The mass and radius of the M-dwarf in the short period eclipsing binary RR Caeli Authors: P.F.L. Maxted (1,2), D. O'Donoghue (3), L. Morales-Rueda (4,2), R. Napiwotzki (5) ((1)Keele University, UK, (2)Southampton University, UK, (3) SAAO, South Africa, (4) Universi...	Blobrana	1	Jan 23 12:46 2012 by Blobrana
	Young moving groups (Preview) Title: Cool Young Stars in the Northern Hemisphere: Beta Pictoris and AB Doradus Moving Group Candidates Authors: Joshua E. Schlieder, Sébastien Lépine, Michal Simon As part of our continuing effort to identify new, low-mass members of nearby, young moving groups (NYMGs), we present a list of y...	Blobrana	0	Jan 20 10:22 2012 by Blobrana
	XB1832-330 (Preview) Title: XMM-Newton observations of the low-mass X-ray binary XB1832-330 in the galactic globular cluster NGC 6652 Authors: L. Sidoli (1), N. La Palombara (1), T. Oosterbroek (2), A.N. Parmar (3) ((1)-INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica, Milano, Italy (2)-Science Payload a...	Blobrana	1	Jan 20 02:37 2012 by Blobrana
	Dwarf nova QZ Virgo Nova (Preview) The dwarf nova QZ Virgo (= T Leo) is in outburst. Date: 2009 01 26 Magnitude: 10.2 - 15.7 Period: ? Satellite period: unknown Type: UGSU Position(2000): RA=11 38 26.82, Dec=+03°22'07.1"	Blobrana	3	Jan 20 05:38 2012 by Blobrana
	OH 231.84 +4.22 (Preview) Title: Rotten Egg Nebula: The magnetic field of a binary evolved star Authors: M. L. Leal-Ferreira, W. H. T. Vlemmings, P. J. Diamond, A. Kemball, N. Amiri, J.-F. Desmurs Most of PNe are not spherical. The loss of spherical symmetry occurs somewhere between the AGB and PN phase. The cause of this chan...	Blobrana	0	Jan 19 18:24 2012 by Blobrana
	U Herculis (Preview) Maximum of U Herculis Variable Star, at 0.6h, 22nd February, 2010 Magnitude=6.4mag Minimum=13.4mag Period= 2.1days Position(2000): RA =16 25 47.4713, Dec =+18 53 32.867	Blobrana	4	Jan 18 00:05 2012 by Blobrana
	G28.87+0.07 (Preview) Title: Massive star-formation toward G28.87+0.07 (IRAS 18411-0338) investigated by means of maser kinematics and radio to infrared, continuum observations Authors: J. J. Li, L. Moscadelli, R. Cesaroni, R. S. Furuya, Y. Xu, T. Usuda, K. M. Menten, M. Pestalozzi, D. Elia, E. Schisano We used the V...	Blobrana	0	Jan 17 03:34 2012 by Blobrana
	UGPSJ0722-05 Sub-brown dwarf (Preview) UGPSJ0722-05 is a sub-brown dwarf located approximately nine light years from Earth. The astronomical object was discovered by Philip Lucas at the University of Hertfordshire in 2010. Read more	Blobrana	5	Jan 17 03:15 2012 by Blobrana
	CW Monocerotis (Preview) The grazing eclipsing dwarf nova CW Monocerotis is in outburst. Date: 27th October 2008 Magnitude: 11.9 - 16.3 Period: 121.7 days Satellite period: 0.1766 days Type: UGSS Position(2000): RA=06 36 54.58, Dec=+00°02'17.2"	Blobrana	2	Jan 16 23:04 2012 by Blobrana
	HX Pegasi (Preview) Date of outbreak: 9th June 2010 Magnitude: 12.9 - 16.62 V Period: 0.2008 days Orbital period of satellite: days Type: UGZ Position(2000): RA=23 40 23.70, Dec=+12°37'41.7"	Blobrana	3	Jan 15 18:45 2012 by Blobrana
	Red giants ( 1 2 ) (Preview) When stars like our sun die, they bloat to become red giants and then eject gigantic clouds of gas and dust into space. Increasingly, however, scientists found themselves at a profound loss to explain how exactly dying stars could blow away these clouds. Now astrophysicists propose that unexpecte...	Blobrana	11	Jan 14 14:11 2012 by Blobrana
	CRTS survey (Preview) Astronomers Release an Unprecedented Data Set on Variability of Celestial Objects An example of a star that flares occasionally. This is a so-called dwarf nova, a binary star system where a material flows from a red giant star to a compact, dense white dwarf companion, and sometimes causes major e...	Blobrana	1	Jan 13 14:50 2012 by Blobrana
	RT Sagittarii (Preview) Maxima of long period variable RT Sagittarii on the 29th April, 2010 Magnitude: 7.0-13.3 V Type: Mira Position (2000): RA 20 17 43.6461, Dec -39 06 46.024	Blobrana	1	Jan 12 00:04 2012 by Blobrana
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