Charles Daney

49 posts · 23,148 views

I'm a science writer interested in most fields of science, and exploring how to make better use of the online environment for providing scientific information to a curious, engaged, but not specialized audience.

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  • February 8, 2012
  • 10:00 PM
  • 50 views

How did some early black holes get so big so fast?

by Charles Daney in Today's Science

The supermassive black holes (SMBHs) found in the centers of large galaxies can be astonishingly large. The closest example to us is in the giant elliptical galaxy M87, and it’s estimated to be 6.6 billion solar masses (M⊙). More distant examples can be even larger, more than 10 billion M⊙ (at distances ~300 million light-years). [...]... Read more »

Di Matteo, T., Khandai, N., DeGraf, C., Feng, Y., Croft, R., Lopez, J., & Springel, V. (2012) COLD FLOWS AND THE FIRST QUASARS. The Astrophysical Journal, 745(2). DOI: 10.1088/2041-8205/745/2/L29  

  • January 30, 2012
  • 02:30 AM
  • 78 views

How large were the first stars in the universe?

by Charles Daney in Today's Science

Since it is currently, and for the foreseeable future, not possible to actually observe what the first stars in the universe were like when they formed, the only way to answer this question is by detailed calculations from first principles. In other words, by computer simulations. Until very recently, such simulations couldn’t be very conclusive, [...]... Read more »

  • January 7, 2012
  • 08:45 PM
  • 110 views

A hyperactive young galaxy

by Charles Daney in Today's Science

Active galaxies contain a supermassive black hole (SMBH) that causes vigorous radiation of electromagnetic energy as a result of rapid accretion of gas and dust. While almost all galaxies except dwarfs contain an SMBH in the center, active galaxies are rare – fewer that 1% of galaxies in the present universe. A very few active [...]... Read more »

  • January 5, 2012
  • 01:30 AM
  • 111 views

Some supermassive black holes are much more super than others

by Charles Daney in Today's Science

Supermassive black holes (SMBHs) can get to be pretty large. Astrophysicists don’t really know what the upper limit is, if any. But before some recent research, the mass of the largest SMBH yet determined was 6.3×109 M⊙ (solar masses). That value is known fairly precisely, since the SMBH is in the nearby giant elliptical galaxy [...]... Read more »

McConnell, N., Ma, C., Gebhardt, K., Wright, S., Murphy, J., Lauer, T., Graham, J., & Richstone, D. (2011) Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies. Nature, 480(7376), 215-218. DOI: 10.1038/nature10636  

  • December 23, 2011
  • 07:04 PM
  • 146 views

Cosmic rays from stellar superbubbles

by Charles Daney in Today's Science

Cosmic rays were discovered almost 100 years ago (1912), yet astrophysicists are still uncertain about where they come from or how they acquire their extremely high energies. Research recently published gives strong evidence that the Cygnus X region, which contains hundreds of very hot, massive, young stars, is a source of cosmic rays and has [...]... Read more »

Ackermann, M., Ajello, M., Allafort, A., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Belfiore, A., Bellazzini, R., Berenji, B.... (2011) A Cocoon of Freshly Accelerated Cosmic Rays Detected by Fermi in the Cygnus Superbubble. Science, 334(6059), 1103-1107. DOI: 10.1126/science.1210311  

  • December 19, 2011
  • 06:30 PM
  • 216 views

Possible constraints on dark matter particle mass

by Charles Daney in Today's Science

Although there is very good indirect evidence for the existence of dark matter, it’s an understatement to say that actual detection of dark matter particles has not been easy. Recent research results from two different teams that both studied gamma rays from dwarf galaxy neighbors of the Milky Way provide an illustration of the difficulty. [...]... Read more »

  • December 11, 2011
  • 11:55 PM
  • 393 views

Active star-forming galaxies have substantial halos

by Charles Daney in Today's Science

Detailed new research shows that there is a distinct correlation between galaxies with large, oxygen-rich gas halos and active ongoing star formation. Although active star formation requires large amounts of available gas, what is surprising is that much, or perhaps even most, of the gas may be in the halo region outside of where most [...]... Read more »

Tumlinson, J., Thom, C., Werk, J., Prochaska, J., Tripp, T., Weinberg, D., Peeples, M., O'Meara, J., Oppenheimer, B., Meiring, J.... (2011) The Large, Oxygen-Rich Halos of Star-Forming Galaxies Are a Major Reservoir of Galactic Metals. Science, 334(6058), 948-952. DOI: 10.1126/science.1209840  

  • December 4, 2011
  • 11:30 PM
  • 126 views

Cygnus X-1 mass and spin determined

by Charles Daney in Today's Science

Cygnus X-1 was a very puzzling object when it was discovered in 1964, because (as the name suggests) it was an extremely powerful X-ray source. Since X-rays are (fortunately) blocked by the Earth’s atmosphere, the exceptional nature of the object was only recognized when it became possible to do astronomy from above the atmosphere, in [...]... Read more »

Reid, M., McClintock, J., Narayan, R., Gou, L., Remillard, R., & Orosz, J. (2011) THE TRIGONOMETRIC PARALLAX OF CYGNUS X-1. The Astrophysical Journal, 742(2), 83. DOI: 10.1088/0004-637X/742/2/83  

Orosz, J., McClintock, J., Aufdenberg, J., Remillard, R., Reid, M., Narayan, R., & Gou, L. (2011) THE MASS OF THE BLACK HOLE IN CYGNUS X-1. The Astrophysical Journal, 742(2), 84. DOI: 10.1088/0004-637X/742/2/84  

Gou, L., McClintock, J., Reid, M., Orosz, J., Steiner, J., Narayan, R., Xiang, J., Remillard, R., Arnaud, K., & Davis, S. (2011) THE EXTREME SPIN OF THE BLACK HOLE IN CYGNUS X-1. The Astrophysical Journal, 742(2), 85. DOI: 10.1088/0004-637X/742/2/85  

  • December 3, 2011
  • 01:37 AM
  • 153 views

Star formation and molecular clouds in the Large Magellanic Cloud

by Charles Daney in Today's Science

The Large Magellanic Cloud (LMC) is the largest close neighbor of our own galaxy, at a distance of only 160,000 light-years – less than twice the diameter of the Milky Way itself. Its proximity makes it a very useful object to study in connection with the process of star formation, which is generally assumed to [...]... Read more »

Wong, T., Hughes, A., Ott, J., Muller, E., Pineda, J., Bernard, J., Chu, Y., Fukui, Y., Gruendl, R., Henkel, C.... (2011) THE MAGELLANIC MOPRA ASSESSMENT (MAGMA). I. THE MOLECULAR CLOUD POPULATION OF THE LARGE MAGELLANIC CLOUD. The Astrophysical Journal Supplement Series, 197(2), 16. DOI: 10.1088/0067-0049/197/2/16  

  • December 1, 2011
  • 11:19 PM
  • 165 views

Magnetic fields may set the stage for birth of new stars

by Charles Daney in Today's Science

Star formation does not happen as easily as one might suppose from the abundance of stars in a galaxy like the Milky Way, in which more than 100 billion times the mass of the Sun (M⊙) exists in the form of stars. Stars condense out of interstellar gas within the galaxy, but the process is [...]... Read more »

  • November 22, 2011
  • 01:00 AM
  • 158 views

Neutron star research points to different classes of supernovae

by Charles Daney in Today's Science

Classifying things is the starting point for almost all scientific fields – from flowers to fundamental particles. Once one has classes the next step is to find subclasses, and then sub-subclasses. Finding correlations between different classification schemes, then, often leads to significant understandings. Neutron stars are not stars in the normal sense. They are remnants [...]... Read more »

  • November 11, 2011
  • 11:00 PM
  • 233 views

Galaxy interactions accelerate the growth of supermassive black holes

by Charles Daney in Today's Science

It’s now well-known that there’s a rough correlation between a galaxy’s size and the size of its central supermassive black hole (SMBH). The correlation is even better (for spiral galaxies) between the black hole size and the size of the central bulge of the galaxy. It’s been found that the mass of a SMBH is [...]... Read more »

J. D. Silverman, P. Kampczyk, K. Jahnke, R. Andrae, S. Lilly, M. Elvis, F. Civano, V. Mainieri, C. Vignali, G. Zamorani.... (2011) The impact of galaxy interactions on AGN activity in zCOSMOS. Astrophysical Journal. arXiv: 1109.1292v1

  • November 8, 2011
  • 11:30 PM
  • 197 views

Hubble directly observes the disk around a black hole

by Charles Daney in Today's Science

Quasars are the brightest persistent objects in the universe. They represent the brightest examples of a somewhat more common object: an active galactic nucleus (AGN). As the name implies, an AGN exists at the center of some galaxies. Most quasars, and even most AGN, are not found in the nearby universe, since they are especially [...]... Read more »

Muñoz, J., Mediavilla, E., Kochanek, C., Falco, E., & Mosquera, A. (2011) A STUDY OF GRAVITATIONAL LENS CHROMATICITY WITH THE HUBBLE SPACE TELESCOPE . The Astrophysical Journal, 742(2), 67. DOI: 10.1088/0004-637X/742/2/67  

  • November 5, 2011
  • 12:43 AM
  • 204 views

Record-breaking gamma-ray emissions from a millisecond pulsar

by Charles Daney in Today's Science

Breaking old records for some statistic or another generally makes for catchy headlines, at least. If nothing else, the fact that the statistic is being tracked (whether or not by Guinness) suggests it’s a matter of more than passing interest. Now astrophysicists have come up with a new find that breaks three records at the [...]... Read more »

, ., Freire, P., Abdo, A., Ajello, M., Allafort, A., Ballet, J., Barbiellini, G., Bastieri, D., Bechtol, K., Bellazzini, R.... (2011) Fermi Detection of a Luminous γ-Ray Pulsar in a Globular Cluster. Science. DOI: 10.1126/science.1207141  

  • October 30, 2011
  • 04:39 AM
  • 221 views

Astronomers Pin Down Galaxy Collision Rate

by Charles Daney in Today's Science

Galaxies have been growing over most of the 13.7 billion year history of the universe. Some of the growth is due to intergalactic gas gradually swept up by an existing galaxy and then driving star formation in the galaxy. But another growth mechanism is the merger of two (and sometimes more) existing galaxies into one. [...]... Read more »

Jennifer M. Lotz, Patrik Jonsson, T. J. Cox, Darren Croton, Joel R. Primack, Rachel S. Somerville, & Kyle Stewart. (2011) The Major and Minor Galaxy Merger Rates at z . Astrophysical Journal. arXiv: 1108.2508v1

  • October 20, 2011
  • 06:30 PM
  • 168 views

Distant Galaxies Reveal The Clearing of the Cosmic Fog

by Charles Daney in Today's Science

The first billion years after the big bang (out of about 13.7 billion years total since then) were among the most interesting in terms of giving birth to the kind of objects that still dominate the scene today. Mostly that means stars and galaxies, plus a few exotica such as quasars. Unfortunately, it’s very difficult [...]... Read more »

L. Pentericci, A. Fontana, E. Vanzella, M. Castellano, A. Grazian, M. Dijkstra, K. Boutsia, S. Cristiani, M. Dickinson, E. Giallongo.... (2011) Spectroscopic confirmation of z~7 LBGs: probing the earliest galaxies and the epoch of reionization. Astrophysical Journal. arXiv: 1107.1376v1

  • October 17, 2011
  • 05:25 PM
  • 222 views

Universe’s “Standard Candles” Are White Dwarf Mergers

by Charles Daney in Today's Science

Supernovae are spectacular but fairly rare events, at least on the human time scale. In our own galaxy, only 5 have been seen (necessarily by the naked eye, before telescopes were invented in 1608) in the last 2000 years. Since there have been none in our galaxy when any telescopes were available to study them, [...]... Read more »

Graur, O., Poznanski, D., Maoz, D., Yasuda, N., Totani, T., Fukugita, M., Filippenko, A., Foley, R., Silverman, J., Gal-Yam, A.... (2011) Supernovae in the Subaru Deep Field: the rate and delay-time distribution of Type Ia supernovae out to redshift 2. Monthly Notices of the Royal Astronomical Society, 417(2), 916-940. DOI: 10.1111/j.1365-2966.2011.19287.x  

  • October 11, 2011
  • 08:10 PM
  • 205 views

A subluminous, normal-width lightcurve Type Ia supernova in the middle of nowhere

by Charles Daney in Today's Science

Astrophysicists have gradually been refining a system of classification for supernovae. The most basic characteristic of interest is whether or not there are spectral lines that indicate the presence of hydrogen. If these lines are absent, the supernova is Type I, which implies the progenitor star was rather old and had used up all of [...]... Read more »

Maguire, K., Sullivan, M., Thomas, R., Nugent, P., Howell, D., Gal-Yam, A., Arcavi, I., Ben-Ami, S., Blake, S., Botyanszki, J.... (2011) PTF10ops - a subluminous, normal-width light curve Type Ia supernova in the middle of nowhere. Monthly Notices of the Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2011.19526.x  

  • October 5, 2011
  • 11:02 PM
  • 197 views

Galaxy Clusters Validate Einstein’s Theory – and Dark Matter Too

by Charles Daney in Today's Science

The theory of relativity – both special relativity and general relativity – has now been tested successfully so many ways ever since its early days that further tests seem almost redundant. (That little mix-up with superluminal neutrinos to the contrary notwithstanding – since it’s at most a higher order correction, but more likely an error [...]... Read more »

  • February 27, 2011
  • 10:26 PM
  • 343 views

Telomerase can reverse the aging process... sort of

by Charles Daney in Science and Reason

Biologists are, at long last, beginning to understand the molecular processes responsible for aging in complex (multicellular) organisms – and to investigate ways to counteract these processes. We discussed one line of research in this recent article about a particular sirtuin (SIRT3) that helps relieve oxidative stress that can lead to DNA damage, which generally leads, in turn, to cell senescence or death.While oxidative stress is certainly a significant factor in aging, possibly the most significant, there are others. One of these is the limitation on a cell's ability to undergo cell division in order to produce new cells of the same type. This is especially important in tissues that regularly need to regenerate, such as skin and intestinal tissue. Everyone now knows about telomeres, whose main function is to constitute protective end caps on chromosomes. The limitation on number of cell divisions happens since about 100 base pairs are lost from telomeres during each cell division. When telomeres eventually become too short signals that are similar to those associated with other kinds of DNA damage shut down a cell's ability to divide further. This mechanism indirectly helps mitigate the risks of DNA damage that are present every time a cell divides – an inherently tricky process.However, this limitation on cell division isn't acceptable during embryonic development, when an organism's cell count is doubling most rapidly. So evolution has provided an enzyme – telomerase – that can rebuild telomeres, but is most active only during embryonic development. Except, of course, in cells that have become cancerous, where the ability to divide without limit is the name of the game. We discussed telomeres and telomerase in some detail a little over a year ago in this article, so you can go there for more.Because of the risk of cancer, it seems imprudent to reactivate telomerase for the long term within an organism, especially in long-lived animals such as humans. (In animals like mice, which live fast and die young, it's a different matter. Telomerase may remain somewhat active in mice during adulthood. (Mentioned here.)) But what if it were possible to reactivate telomerase for a relatively short period of time (compared to the whole lifespan)... might that provide an opportunity to rebuild telomeres to some extent? Even better, might that reverse, at least to some extent, the ravages of aging?We now have some research that seems to provide a fairly unambiguous affirmative answer... in a rather special case: Telomerase reactivation reverses tissue degeneration in aged telomerase-deficient mice. But didn't we just say that mice may retain telomerase activity throughout their lives? Yes, however it's a relatively simple matter to "knock out" the main telomerase gene in mice (Tert). When that's done the resulting strain of knock-out mice – after several generations – have shortened lifespans and a general phenotype of age-related debilities, as one would expect. (The first few generations apparently still have sufficiently long teleomeres.) Unfortunately, that's not a good enough model, since without a Tert gene, the organism has no way to manufacture telomerase. Simply giving the knock-out mice repeated infusions of telomerase is not a good way to ensure uniform distribution of the enzyme to all of the organism's cells. What to do? The experimenters came up with a rather clever solution. Normally the way that telomerase is activated in cells is by means of an "estrogen receptor" (ER), to which a form of the hormone estrogen (17β-estradiol to be precise) can bind and enable transcription of Tert. This ER can be tweaked so that estrogen binds to it only in the presence of another chemical, 4-hydroxytamoxifen (4-OHT). A special form of the Tert gene that includes this special ER can be "knocked-in" to the mouse germline. It then turns out that 4-OHT can be efficaciously supplied to a TERT-ER mouse (in the form of a time-release subcutaneous pellet) to turn telomerase expression on and off at the experimenter's will. With that technology in place, the researchers were then able to perform a series of experiments demonstrating, in these special mice, that a month-long burst of telomerase could actually reverse a number of the ill effects of telomerase deprivation.The first step was to show that without 4-OHT the TERT-ER mice (after a few generations) had many of the same problems, in the same degree, as later generations of knock-out mice that lacked Tert entirely. The TERT-ER mice (all of which were male) showed no signs of telomerase activity. Tissues in highly proliferative organs such as testes, spleen, and intestines showed notable atrophy. Lifespan of TERT-ER mice was about half that of normal ("wild type") mice.The first test to investigate the effects of telomerase reactivation by means of 4-OHT was done in vitro. Fibroblast cells from TERT-ER mice were cultured and found to be essentially senescent and not undergoing cell cycles. But when the cells were placed in media containing 4-OHT, teleomerase was reactivated, telomeres lengthened, and cell proliferation resumed.Some TERT-ER mice were then given a 4-week treatment of 4-OHT (subcutaneous pellets). At the end of that treatment there was a marked reversal of the degeneration that has occurred in testes, spleen, liver, and intestinal tissues, as well as resumption of sperm production. Survival time of these treated mice also increased. At the same time, 4-OHT had no effects on control mice that weren't lacking in telomerase and didn't have tissue degeneration.Noteworthy results were obtained from tests to assess nervous system condition. Proliferation of neural progenitor cells was found to resume in TERT-ER mice treated with 4-OHT. Normal numbers of mature oligodendrocytes reappeared. Lastly, high-level neurological functions were restored, as indicated by resumption of nearly normal olfactory sensitivity.An interesting conclusion that can be drawn from the neurological results is that neural progenitor cells probably survive loss of telomeres, so that they can rebuild neural cell populations if telomeres are repaired.The really interesting question, of course, is the extent to which these results may apply, in some form, to humans. Unfortunately, there are a number of reasons to be skeptical. For one thing, telomere shortening is only one factor, and quite possibly not the main one, in human aging. Aging can be thought of as a complex disease, like cancer, with many contributing factors. The consequences of telomere truncation are only one factor.Further, murine biology has signficant differences from human biology. Mice are less complex organisms, with rather short lifespans. Mice seem to retain some degree of telomerase activity throughout their lives, so they are not as well adapted to going for long periods without it.It is noteworthy that evidence was not found that TERT-ER mice treated with 4-OHT became more susceptible to cancer. Still, mice don't live very long, and they are adapted to maintain active telomerase. Humans are different. If telomerase is artificially kept active for years in humans, incipient tumorigenicity could be accelerated.Lastly, it's not necessarily easy to raise human telomerase activity levels in the first place. Although some telomerase-activating factors are known, they have not been tested extensively in humans for long periods of time, so their safety and efficacy profile is not known.These research results are quite interesting – but they only indicate the need for much more investigation.... Read more »

Jaskelioff, M., Muller, F., Paik, J., Thomas, E., Jiang, S., Adams, A., Sahin, E., Kost-Alimova, M., Protopopov, A., Cadiñanos, J.... (2010) Telomerase reactivation reverses tissue degeneration in aged telomerase-deficient mice. Nature, 469(7328), 102-106. DOI: 10.1038/nature09603  

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