* Astronomy

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Maxima of long period variable Y Pegasi on the 4th March, 2010 Magnitude: 10.5-14.9 Type: Mira Position (2000): RA 22 11 37.5, Dec +14 21 56

Blobrana · Blobrana

The SU UMa-type cataclysmic variable SW UMa is in superoutburst. The last time the star was in outburst, in October 2002, it reached visual magnitude 10.5 and was brighter than 13.5 for 17 days. The normal minimum magnitude is approxim...

Blobrana · Blobrana

Title: WASP-14b: A 7.7 Mjup transiting exoplanet in an eccentric orbit Authors: Y. C. Joshi, D. Pollacco, A. Collier Cameron, I. Skillen, E. Simpson, I. Steele, R. A. Street, H. C. Stempels, F. Bouchy, D. J. Christian, N. P. Gibson, L. Hebb, G. Hebrard, F. P. Keenan, B. Loeillet, J. Meaburn, C...

Blobrana · Blobrana

Title: Why are central radio relics so rare? Authors: F. Vazza, M. Brueggen, R. van Weeren, A. Bonafede, K. Dolag, G. Brunetti In this paper we address the question why cluster radio relics that are connected to shock acceleration, so-called radio gischt, have preferentially been found in the outs...

Blobrana · Blobrana

Title: The variability of the CoRoT target HD171834: gamma Dor pulsations and/or activity? Authors: K. Uytterhoeven, P. Mathias, A. Baglin, M. Rainer, E. Poretti, P. Amado, E. Chapellier, L. Mantegazza, K. Pollard, J. C. Suarez, P. M. Kilmartin, K. H. Sato, R. A. Garcia, M. Auvergne, E. Michel, R....

Blobrana · Blobrana

Maxima of long period variable RY Ophiuchi on the 15th March, 2010 Magnitude: 7.4 - 13.8 V Type: Mira Period: 150.41 days Position (2000): RA 18 16 36.9363, Dec +03 41 35.346

Blobrana · Blobrana

Title: A Monte Carlo analysis of the velocity dispersion of the globular cluster Palomar 14 Authors: A. Sollima, C. Nipoti, A. Mastrobuono Battisti, M. Montuori, R. Capuzzo-Dolcetta We present the results of a detailed analysis of the projected velocity dispersion of the globular cluster Palom...

Blobrana · Blobrana

Maxima of long period variable X Camelopardalis on the 8th April, 2010 Magnitude: 8.1-12.6 V Type: Mira Position (2000): RA 04 45 42.1935, Dec +75 06 03.465

Blobrana · Blobrana

Maxima of long period variable V Virginis on the 1st July, 2010 Magnitude: 8.9-14.3 Type: Mira Position (2000): RA 13 27 48.1471, Dec -03 10 22.881

Blobrana · Blobrana

Title: Massive black holes lurking in Milky Way satellites Authors: S. Van Wassenhove, M. Volonteri, M.G. Walker, J.R. Gair As massive black holes (MBHs) grow from lower-mass seeds, it is natural to expect that a leftover population of progenitor MBHs should also exist in the present universe. Dw...

Blobrana · Blobrana

A small, dense object only twelve miles in diameter is responsible for a beautiful X-ray nebula that spans 150 light years. At the center of a new image made by NASA's Chandra X-ray Observatory is a very young and powerful pulsar, known as PSR B1509-58, or B1509 for short. The pulsar is a rapidly spinni...

Blobrana · Blobrana

Title: Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region Authors: Fumitaka Nakamura (NAOJ), Tomoya Miura (Niigata Univ.), Yoshimi Kitamura (JAXA), Yo****o Shimajiri (NRO), Ryohei Kawabe (NRO), Norio Ikeda (JAXA), Takashi Tsukagoshi (Univ. of...

Blobrana · Blobrana

[url=http://www.activeboard.com/forum.spark?forumID=58381&subForumID=150691&action=viewTopic&commentID=3273659]Smal...

Blobrana · Blobrana

Zeta Aurigae is a star in the constellation Auriga. It has traditional names Haedus (also Hoedus) and Sadatoni (rarely Saclateri). Zeta Aurigae is an Algol type eclipsing binary, which varies from magnitude +3.61 to +3.99 with a period of 972 days. The main star is a red K5II supergiant, the blue B7V...

Blobrana · Blobrana

The U Gem type variable star KX Aquilae is in outburst The dwarf nova was observed by T. Gomez (Madrid) at magnitude 13.58 on the 9th March 2010. Position (2000): RA 19 33 53.686, Dec +14 17 47.30

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	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
	Y Pegasi Mira (Preview) Maxima of long period variable Y Pegasi on the 4th March, 2010 Magnitude: 10.5-14.9 Type: Mira Position (2000): RA 22 11 37.5, Dec +14 21 56	Blobrana	1	Nov 15 00:02 2011 by Blobrana
	SW Ursae Majoris (Preview) The SU UMa-type cataclysmic variable SW UMa is in superoutburst. The last time the star was in outburst, in October 2002, it reached visual magnitude 10.5 and was brighter than 13.5 for 17 days. The normal minimum magnitude is approxim...	Blobrana	1	Nov 12 22:53 2011 by Blobrana
	WASP-14b extrasolar planet Exoplanet (Preview) Title: WASP-14b: A 7.7 Mjup transiting exoplanet in an eccentric orbit Authors: Y. C. Joshi, D. Pollacco, A. Collier Cameron, I. Skillen, E. Simpson, I. Steele, R. A. Street, H. C. Stempels, F. Bouchy, D. J. Christian, N. P. Gibson, L. Hebb, G. Hebrard, F. P. Keenan, B. Loeillet, J. Meaburn, C...	Blobrana	2	Nov 11 11:49 2011 by Blobrana
	Radio Relics (Preview) Title: Why are central radio relics so rare? Authors: F. Vazza, M. Brueggen, R. van Weeren, A. Bonafede, K. Dolag, G. Brunetti In this paper we address the question why cluster radio relics that are connected to shock acceleration, so-called radio gischt, have preferentially been found in the outs...	Blobrana	0	Nov 9 10:03 2011 by Blobrana
	HD171834 (Preview) Title: The variability of the CoRoT target HD171834: gamma Dor pulsations and/or activity? Authors: K. Uytterhoeven, P. Mathias, A. Baglin, M. Rainer, E. Poretti, P. Amado, E. Chapellier, L. Mantegazza, K. Pollard, J. C. Suarez, P. M. Kilmartin, K. H. Sato, R. A. Garcia, M. Auvergne, E. Michel, R....	Blobrana	0	Nov 9 09:59 2011 by Blobrana
	RY Ophiuchi Mira (Preview) Maxima of long period variable RY Ophiuchi on the 15th March, 2010 Magnitude: 7.4 - 13.8 V Type: Mira Period: 150.41 days Position (2000): RA 18 16 36.9363, Dec +03 41 35.346	Blobrana	1	Nov 9 00:01 2011 by Blobrana
	Palomar 14 Globular clusters Palomar (Preview) Title: A Monte Carlo analysis of the velocity dispersion of the globular cluster Palomar 14 Authors: A. Sollima, C. Nipoti, A. Mastrobuono Battisti, M. Montuori, R. Capuzzo-Dolcetta We present the results of a detailed analysis of the projected velocity dispersion of the globular cluster Palom...	Blobrana	0	Nov 8 10:16 2011 by Blobrana
	X Camelopardalis (Preview) Maxima of long period variable X Camelopardalis on the 8th April, 2010 Magnitude: 8.1-12.6 V Type: Mira Position (2000): RA 04 45 42.1935, Dec +75 06 03.465	Blobrana	2	Nov 6 00:32 2011 by Blobrana
	V Virginis Mira (Preview) Maxima of long period variable V Virginis on the 1st July, 2010 Magnitude: 8.9-14.3 Type: Mira Position (2000): RA 13 27 48.1471, Dec -03 10 22.881	Blobrana	1	Nov 5 00:03 2011 by Blobrana
	Massive black holes Blackholes (Preview) Title: Massive black holes lurking in Milky Way satellites Authors: S. Van Wassenhove, M. Volonteri, M.G. Walker, J.R. Gair As massive black holes (MBHs) grow from lower-mass seeds, it is natural to expect that a leftover population of progenitor MBHs should also exist in the present universe. Dw...	Blobrana	7	Nov 1 08:24 2011 by Blobrana
	PSR B1509-58 (Preview) A small, dense object only twelve miles in diameter is responsible for a beautiful X-ray nebula that spans 150 light years. At the center of a new image made by NASA's Chandra X-ray Observatory is a very young and powerful pulsar, known as PSR B1509-58, or B1509 for short. The pulsar is a rapidly spinni...	Blobrana	5	Nov 1 08:11 2011 by Blobrana
	L1641-N Region (Preview) Title: Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region Authors: Fumitaka Nakamura (NAOJ), Tomoya Miura (Niigata Univ.), Yoshimi Kitamura (JAXA), Yo****o Shimajiri (NRO), Ryohei Kawabe (NRO), Norio Ikeda (JAXA), Takashi Tsukagoshi (Univ. of...	Blobrana	0	Oct 31 02:37 2011 by Blobrana
	NGC346 ( 1 2 ) Milky Way NGC (Preview) [url=http://www.activeboard.com/forum.spark?forumID=58381&subForumID=150691&action=viewTopic&commentID=3273659]Smal...	Blobrana	12	Oct 31 01:58 2011 by Blobrana
	zeta Aurigae (Preview) Zeta Aurigae is a star in the constellation Auriga. It has traditional names Haedus (also Hoedus) and Sadatoni (rarely Saclateri). Zeta Aurigae is an Algol type eclipsing binary, which varies from magnitude +3.61 to +3.99 with a period of 972 days. The main star is a red K5II supergiant, the blue B7V...	Blobrana	3	Oct 29 21:30 2011 by Blobrana
	KX Aquilae (Preview) The U Gem type variable star KX Aquilae is in outburst The dwarf nova was observed by T. Gomez (Madrid) at magnitude 13.58 on the 9th March 2010. Position (2000): RA 19 33 53.686, Dec +14 17 47.30	Blobrana	2	Oct 28 13:21 2011 by Blobrana
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